The galaxy appears to be a relatively smooth, elliptical-type galaxy, presenting a somewhat regular and amorphous structure. The core exhibits a brighter, more concentrated region that gradually fades into the outer regions. The overall color profile shows a bias towards the redder end of the spectrum, indicative of an older stellar population and lower current star formation rate. There is some indication of a possible minor interaction or tidal disturbance, visible as a faint, asymmetric extension on one side. The galaxy's shape is primarily in between round and cigar shaped.
