This galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a central bulge that is very bright and concentrated, with the intensity of light decreasing gradually toward the outer edges. The overall shape is noticeably elongated but not excessively so, appearing mostly circular. There is a hint of a disk-like structure, though this is not very distinct, and no spiral arm features are visible. The galaxy is fairly isolated with no signs of interaction or recent merging events. Color gradients are subtle, with the central bulge appearing slightly more yellow/white, transitioning to a bluer hue in the outskirts. The overall low star formation rate is consistent with the observed morphology, suggesting a population dominated by older stars.
