The galaxy presents as a concentrated object with an elliptical morphology. The central region appears bright and yellow. The light distribution from the core outwards gradually decreases in intensity. It exhibits a smooth overall appearance with no obvious spiral arm structures or prominent dust lanes. A slight asymmetry may be present, with a possible subtle extension on one side. The color profile suggests a predominantly older stellar population. There is no indication of ongoing major merger activity, although subtle disturbances cannot be ruled out.
