This galaxy presents as a fairly compact, disk-like structure with an apparent diameter of approximately 3.6 arcseconds. The central region exhibits a bright, concentrated luminosity profile, suggesting the presence of a prominent galactic bulge. The inner disk appears relatively smooth and featureless, displaying a consistent color gradient moving outward from the center. The outer regions of the disk show some signs of faint, irregular structure, potentially indicative of tidal interactions or minor disturbances. Overall, the galaxy exhibits a flattened morphology, but with a substantial bulge component. There are a few hints of asymmetry in the outer disk, which might imply some past or ongoing gravitational interaction. It does not appear to be undergoing a major merger. 
