The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a rounded morphology, appearing more circular than elongated. The light distribution suggests a dominant bulge component, with a gradual decrease in surface brightness outward from the core.

The color gradient is subtle but discernable. The central region appears more yellow, possibly indicative of an older stellar population. The outer regions show a slightly bluer tint, potentially reflecting the presence of younger stars, although this is not highly pronounced. There is no clear evidence of spiral arm structure or significant dust lanes.

Based on these observations, this galaxy is likely an elliptical galaxy, possibly of intermediate mass. The lack of significant features suggestive of active star formation may point to a relatively passive evolutionary state. Further spectroscopic data would be needed to confirm its exact classification and star formation history.
