The galaxy presents an edge-on disc morphology. A prominent bulge is visible, exhibiting a smooth profile, and appears to be slightly elongated. The dust lane is clearly observed, bisecting the galaxy along its major axis. The stellar disk extends significantly beyond the bulge, showing a gradual fading in luminosity towards its edges. The galaxy has a moderately high surface brightness, with the bulge being the brightest region, exhibiting a yellowish-orange hue. The disk appears bluer, suggesting the presence of ongoing star formation. The overall color index indicates a relatively evolved stellar population, with a noticeable contribution from younger stars in the disk. There is no obvious evidence of a tidal disturbance or recent merger activity.
