This galaxy presents as a relatively small, yet moderately luminous object, displaying a distinct disk-like morphology viewed nearly edge-on from our vantage point. The central bulge exhibits a bright, concentrated luminosity gradient, with a yellowish-white color suggesting a substantial population of older stars. The bulge appears rounded rather than boxy.

The disk itself is thin and elongated, with a noticeable dust lane bisecting it along the major axis. This obscuration indicates the presence of significant interstellar medium within the galactic plane. The disk shows hints of redder hues along its outer edges, consistent with the presence of older stellar populations or dust extinction.

There is no strong evidence of recent major merger activity or significant tidal disturbances in the immediate vicinity of the galaxy. The overall structure appears relatively undisturbed, aside from minor irregularities within the disk. The galaxy's light profile seems relatively smooth, with a dominance of disk features and a relatively small contribution from spiral arms.

The galaxy's color indices suggest intermediate activity star formation, as the galaxy appears more red and therefore, has more stars in the red wavelength band.
