The galaxy presents as a relatively compact object with a moderately smooth overall appearance. It exhibits a somewhat elliptical shape, appearing more elongated than circular. The light distribution within the galaxy seems predominantly concentrated toward the center, suggestive of a central bulge. 

There is evidence of some form of disturbance, potentially indicative of minor gravitational interactions, but the overall structure does not appear to be highly disrupted. The galaxy displays a range of colors, with the central regions trending towards redder hues, and hints of bluer tints at the outer edges, which may indicate varying stellar populations and regions of differing star formation activity within the galaxy.
