The galaxy presents as a lenticular or edge-on spiral, characterized by a smooth, elongated morphology. It exhibits a high degree of central concentration, suggesting the presence of a significant bulge component. The disk appears relatively thin and uniform in color, with no discernible spiral arm structure visible at this resolution. There are slight hints of a minor disturbance or tidal feature. The galaxy's overall color is indicative of an older stellar population. There is no significant dust lane obscuration apparent.
