The galaxy displays a central bulge that is relatively bright and compact, suggesting a higher concentration of older stellar populations. A disk-like structure surrounds the bulge, appearing relatively smooth with subtle variations in brightness, and the presence of weak spiral arm features, albeit somewhat indistinct. The galaxy's disk is oriented approximately edge-on, hindering a clear view of its spiral structure. The overall color of the galaxy appears reddish, indicative of an evolved stellar population. Some indications of tidal interactions are present, suggesting that minor disturbances are occurring. A faint and distorted tail-like structure extends outwards from the galaxy, possibly resulting from past or ongoing gravitational interactions. The central bulge is dominated by a bright, relatively compact core, indicating potential activity from a supermassive black hole.
