The galaxy presents as a centrally concentrated, relatively smooth, and elliptical-like structure. It exhibits a dominant, bright core region that gradually fades into a more diffuse halo. The color profile suggests an older stellar population, with a yellowish-red hue dominating the central regions. There is no readily apparent spiral arm structure or dust lane obscuration visible. The overall morphology indicates a system that is likely in a relatively advanced stage of its evolution. There are no obvious signs of recent major merger events or significant tidal disturbances. The galaxy appears largely isolated with no clear evidence of immediate interaction with companion galaxies.
