The galaxy presents an overall smooth, elliptical morphology, indicating a classification as an elliptical galaxy. Its light profile suggests a centrally concentrated stellar population, with a gradual decrease in surface brightness towards the outer edges. The galaxy exhibits a yellow-white hue, indicating a population of older stars. No distinct spiral arm structure or dust lanes are apparent, further supporting an elliptical classification. There is a very slight elongation, with an axis ratio close to 1. The galaxy shows no signs of any major interactions or disturbances.
