The galaxy presents as a relatively smooth, centrally concentrated object. There appears to be a dominant, bright bulge component. Some hints of disk structure with faint, diffuse extensions are present beyond the primary bulge. The galaxy exhibits a slightly oblong shape, with a moderate elongation. There is a subtle color gradient, with the central regions appearing more yellow-white, indicating an older stellar population, possibly with higher metallicity. The outer extensions show a slightly bluer tint, potentially representing younger stars or regions of recent star formation. There is a possibility of minor disturbances present, with some asymmetry and hints of tidal features but no strong indication of on-going major mergers. There also appears to be at least two other faint galaxies in close proximity to the main galaxy, which could be interacting with the main one.
