The galaxy presents as a relatively smooth, centrally concentrated object with an elliptical morphology. It appears elongated, with a minor axis approximately half the length of the major axis. The core region exhibits a bright, yellow-white hue, suggesting a dominant population of older stars. This color gradually fades towards the outer edges of the galaxy, indicating a decrease in stellar density. There are slight hints of a disk-like structure but the galaxy is mostly smooth. There is no evidence of significant dust lanes, spiral arms, or active star-forming regions within this object. There is no apparent merging or tidal disruptions. 
