The galaxy presents as a centrally concentrated object with a generally smooth morphology. It appears elliptical in shape, displaying a noticeable but not extreme deviation from circularity. There is a hint of asymmetry in its outer regions, possibly indicative of a minor tidal interaction or internal disturbance. The color gradient suggests a population of older stars dominating the central bulge, with a slight bluer hue in the surrounding areas perhaps indicating a small population of younger stars, albeit with relatively suppressed star formation. Overall, the galaxy appears to be a relatively quiescent system.
