The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. There appears to be two distinct centers of luminosity, suggesting the possibility of an ongoing or recent merger event. The overall color of the galaxy leans towards the redder end of the spectrum, indicating a population dominated by older stars and a relatively low rate of current star formation. The shape appears fairly round and has a relatively compact size. There is a faint hint of possible tidal features or disturbances surrounding the main body, further supporting the hypothesis of a merging system.
