The galaxy presents an elliptical morphology, exhibiting a smooth and somewhat elongated structure. The central region displays a bright, concentrated core that fades gradually towards the outer edges, with a slight tilt, the galaxy demonstrates axial symmetry. The galaxy's color profile indicates a relatively passive stellar population, with redder hues concentrated in the outskirts, suggesting older stars, while the central region exhibits a bluer tint, potentially indicative of younger stars. The overall appearance implies a relatively evolved system, possibly undergoing a period of quiescence in terms of star formation activity. There are some irregularities that may indicate some minor disturbances.
