The galaxy appears to be a relatively smooth, elliptical galaxy with a round morphology. It exhibits a centrally concentrated light profile, gradually decreasing in intensity towards the outer edges. There is a subtle color gradient, transitioning from a slightly bluer hue in the core to a redder hue in the outer regions, indicative of potentially older stellar populations in the galaxy's outskirts. There is no apparent spiral arm structure or distinct features, suggesting an evolved system. No signs of any major mergers or strong tidal disturbances are present.
