The galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated, bright central region that gradually fades into a more diffuse outer halo. The color gradient suggests a population of older stars, contributing to its yellowish-red hue. There is no indication of a prominent disk structure, spiral arms, or significant dust lanes. The overall morphology suggests a relaxed system that is not undergoing a major merger event. There is a very slight hint of a tidal feature to the left of the galaxy.
