The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. The color profile suggests a relatively homogenous stellar population with a dominant yellow-red hue, potentially indicating an older stellar population. The galaxy displays a fairly uniform, diffuse halo with a low surface brightness, gradually fading into the background sky. There is no apparent spiral arm structure or significant dust lane features. The round appearance suggests it is not highly inclined with respect to our line of sight. No prominent tidal features or indications of recent major merger activity are visible. There are no indications of active star formation based on the color profile. 
