The galaxy exhibits a generally smooth, elongated morphology, appearing somewhat cigar-shaped in its overall form. It presents a concentrated central bulge that gradually fades into the outer regions, showing characteristics of an elliptical galaxy.

The color distribution suggests a redder core, which could indicate an older stellar population dominating the galactic center. The outer regions appear slightly bluer, potentially indicating the presence of younger stars, though this bluer component is subdued. There is little evidence of distinct spiral arms or significant dust lanes. Faint irregular structure is present. There appears to be no strong ongoing star formation activity. The overall appearance suggests a system that has largely ceased its major star-forming processes. 
