The galaxy appears as an elongated structure, likely a spiral galaxy viewed edge-on or nearly edge-on. It exhibits a bright, concentrated central bulge, which gradually fades into a fainter, more diffuse disk. The disk appears to be relatively smooth, with limited or poorly resolved spiral arm structures.

The galaxy's color profile suggests a moderate level of star formation. The central bulge appears more yellow-white, indicative of an older stellar population, while the disk shows a slight bluish tint, suggestive of younger, hotter stars associated with ongoing star formation.

Dust lanes are subtly visible within the disk, appearing as dark streaks or patches silhouetted against the brighter starlight. These lanes obscure some of the light from the stars behind them. The galaxy lacks any obvious signs of major disturbances or interactions with other galaxies.
