The galaxy appears as a relatively compact, elliptical-like structure. It exhibits a smooth, centrally concentrated light profile, with the brightest region located near the center. There is a slight elongation, suggesting a deviation from a perfect circular shape. The galaxy's color is predominantly yellowish-orange, indicating a population of older stars. The presence of a merger seems likely, judging by the irregular features and asymmetric light distribution. There are minor disturbances within the galaxy's structure, hinting at possible interactions or past merger events. Some regions show a slightly bluer hue, hinting at the existence of a very small population of younger stars or regions of star formation. Overall, the galaxy appears to be in a relatively quiescent state, with little ongoing star formation.
