The galaxy appears to be an elliptical system, exhibiting a generally smooth morphology. Its light profile suggests a centrally concentrated spheroid with a gradual decline in brightness outwards. The galaxy displays a notable amount of redder light, implying an older stellar population. Indications of a possible ongoing or past merger event are present, characterized by some disturbed light distribution. There is evidence to suggest star formation is currently suppressed. The galaxy is relatively compact in size.
