The galaxy presents as a moderately luminous object with a concentrated central bulge. The overall shape is elliptical, appearing rather smooth and featureless with no discernible spiral arm structure. The color profile suggests a population of older stars, indicated by the reddish-yellow hue of the central bulge. There may be a hint of a slightly bluer, fainter disk surrounding the bulge but this is difficult to discern due to the galaxy's distance and potential obscuration. There is no strong evidence of recent or ongoing major merger activity, although subtle irregularities may indicate past minor interactions.
