The galaxy presents as an elliptical morphology with a smooth, symmetrical light distribution. Its color is predominantly red/yellow, suggestive of an older stellar population. The galaxy appears relatively compact, and there is evidence for a possible ongoing or past merger event given its slightly disturbed morphology and multiple cores. The overall appearance suggests a galaxy that is not currently undergoing significant star formation, supported by the red color. There are minor irregularities in the outer regions, possibly indicative of tidal debris or interactions with smaller galaxies.
