The galaxy presents as a lenticular or edge-on spiral, exhibiting a smooth, elongated morphology indicative of an elliptical shape when viewed face-on. The central bulge is bright and appears yellowish-white in color. Diffuse light extends outwards from the bulge, with some indication of a faint disk. There is a notable lack of distinct spiral arm structure, which, in combination with the smooth appearance, suggests that the galaxy has largely ceased significant star formation. The color gradient indicates that the bulge likely consists primarily of an older stellar population, while the bluer hue along the edges hints at the presence of a young population of stars or gas clouds on the outer edges of the disk. The galaxy's overall morphology shows no major disturbances due to recent major mergers, although some slight asymmetries are seen in the outer disk.
