The galaxy presents as a single, centrally concentrated object with a relatively smooth morphology. It exhibits a luminous core region that gradually diffuses outward, transitioning into a more extended halo. There are subtle variations in color across the galaxy, with the central region appearing more yellowish, potentially indicative of an older stellar population, while the outer regions exhibit a slightly bluer hue. There is no apparent spiral arm structure or significant dust lane obscuration visible. The overall shape is roughly elliptical, but not perfectly spherical, appearing somewhat flattened. There are no signs of recent major mergers or significant tidal disturbances. The light profile suggests that the galaxy is likely an early-type galaxy with a significant spheroidal component.
