The galaxy presents a predominantly smooth morphology, indicative of an elliptical or lenticular type. The color profile suggests a population of older stars. The galaxy exhibits a noticeable central bulge, transitioning smoothly outwards. It has an elongated shape, its major axis noticeably larger than its minor axis, and the object does not appear to have any spiral arm structure or significant dust lanes. There is no apparent active galactic nucleus or ongoing major starburst activity. The object does not exhibit signs of a recent major merger event. 
