The galaxy presents as a fairly smooth, centrally concentrated light distribution with a generally elliptical morphology. The core of the galaxy exhibits a yellowish hue, suggestive of an older stellar population. Fainter, somewhat greenish-blue light is observed in the outer regions, potentially indicative of some ongoing, albeit subdued, star formation activity. There is no distinct spiral arm structure or bar visible. No obvious tidal features or indications of recent major mergers are seen in the image.
