The galaxy presents a generally smooth appearance with a slight asymmetry. The central bulge region exhibits high luminosity, suggesting a dense stellar population. Faint, diffuse disk-like features are present, although not sharply defined. The galaxy appears to be relatively isolated, lacking obvious signs of recent major mergers or interactions. There may be minor disturbances present in the outer regions, which could be suggestive of past or ongoing minor interactions. The overall shape of the galaxy is more rounded than elongated, with a subtle extension toward one side. There is a color gradient, with the central regions appearing bluer than the outer regions.
