The object appears to be a galaxy viewed edge-on. It exhibits a pronounced central bulge that is relatively smooth and concentrated. The disk is quite thin and elongated, with a noticeable difference in color compared to the bulge. The bulge appears to be composed of older stars, exhibiting a redder hue. The disk exhibits a bluer tint, suggesting the presence of younger stars and ongoing star formation. The overall symmetry of the galaxy appears largely undisturbed, though there might be a minor irregularity or faint tidal feature extending from one end of the disk, which could be indicative of a past minor interaction or internal disturbance. The galaxy does not seem to have a prominent dust lane bisecting the disk, although there appears to be some minor obscuration.
