The galaxy presents as a relatively smooth, centrally concentrated object. Its overall morphology appears to be elliptical or lenticular, exhibiting a diffuse, spheroid-like structure with minimal discernible spiral arm features. The core region exhibits a yellowish-white hue, suggesting an older stellar population. Moving outward from the core, the color transitions to a more subtle blue-green, potentially indicative of some ongoing, albeit subdued, star formation in the outer regions. No pronounced dust lanes or significant tidal features are readily apparent, and the overall structure shows no significant distortions, suggesting a dynamically relaxed state. A very slight elongation along one axis can be observed.
