The galaxy presents a predominantly smooth morphology, appearing elliptical in shape. A slight elongation is noticeable, deviating marginally from a perfectly circular form. The central region exhibits a high concentration of light, indicative of a substantial galactic nucleus. The color gradient suggests a population of older stars dominating the galactic composition, with a general reddish-yellow hue. Faint, diffuse features extend from the main body, possibly representing tidal tails or streams of stars. These features are more apparent on one side of the galaxy. Overall, the galaxy appears relatively undisturbed, without signs of a recent major merger.
