The galaxy presents a largely smooth and centralized light distribution, appearing generally elliptical in shape. There is a concentrated central bulge region, exhibiting a slightly redder hue, possibly indicating an older stellar population dominating this area. The outer regions appear fainter and bluer. The disk component, if present, is not well-defined, though there seems to be a slight flattening evident. The overall color suggests that star formation may be ongoing, though at a low rate. There is no strong evidence of recent major mergers or significant tidal disturbances, though there appears to be a minor disturbance. There is a slight asymmetry in the outer regions on one side, but it is unclear if this is a result of interaction. 
