The galaxy presents as a moderately compact, elliptical-like structure. It exhibits a generally smooth morphology with a high degree of central concentration. The overall color appears to be slightly reddish, suggesting an older stellar population. There is no distinct spiral arm structure visible, nor are there any significant dust lanes or prominent star-forming regions discernible. There's a subtle hint of a possible tidal interaction or minor disturbance present, evidenced by a slight asymmetry in the outer isophotes. The roundness is intermediate, and the color suggests a more passive star formation rate and a substantial stellar mass. The light profile appears relatively smooth and undisturbed.
