The galaxy presents with a moderately compact morphology. It displays a bright, concentrated central bulge, potentially indicative of an older stellar population or the presence of an active galactic nucleus. The light profile appears relatively smooth, with only subtle deviations suggesting faint, diffuse structures extending outwards from the central region. Some asymmetry is noticeable, particularly a slight elongation of the galaxy's shape, suggesting a possible interaction or tidal disturbance, however subtle. The outer regions fade rapidly, and the general shape is most likely that of a spiral galaxy viewed from the top down.
