The galaxy presents as a centrally concentrated object with a generally smooth morphology. It exhibits a nearly circular profile. The central region displays a significantly higher surface brightness and a yellowish hue, suggesting an older stellar population dominating the core. There are subtle color variations outwards from the core, however no clear spiral arm or disk-like structures are readily apparent. The outer regions display a more diffuse light distribution, gradually fading into the background sky. Overall, the galaxy appears undisturbed, showing no strong evidence of tidal interactions or major mergers, though there may be a hint of minor disturbances. The light distribution suggests a relatively evolved system, potentially an elliptical or an early-type spiral seen face-on, with a significant bulge component.
