This galaxy exhibits a morphology that suggests an interaction or possible merger. The primary galactic body appears relatively smooth and somewhat elliptical, with a concentrated central bulge exhibiting a yellow hue. Emanating from this central region is a fainter, extended structure or tidal tail, displaying a bluer color indicative of younger stellar populations. This extended feature is suggestive of a gravitational interaction, perhaps with a smaller galaxy that has since been disrupted. The overall shape deviates noticeably from a regular elliptical, supporting the hypothesis of an ongoing or recent disturbance of its morphology. The galaxy is relatively compact. Star formation appears to be suppressed or minimal in the main body, although potentially more active within the tidal feature.
