The galaxy presents a generally smooth, elliptical morphology. The core region exhibits a bright, concentrated luminosity profile, suggesting a high density of stars. The galaxy appears somewhat rounded in shape, with a subtle elongation along one axis. A minor disturbance in the form of a small amount of light extending away from the galaxy may indicate a potential tidal interaction or a subtle merger event in progress. The overall color profile suggests a population of older stars, contributing to the yellowish-orange hue observed. The estimated size suggests a moderate to relatively large galaxy based on luminosity.
