The galaxy exhibits a primarily smooth morphology, with a slightly elongated, elliptical shape. The central region presents a bright, concentrated core, suggesting a high stellar density or possible active galactic nucleus. The color gradient transitions from a yellowish-orange core to a bluer hue towards the outer edges, indicative of a change in stellar population or dust content. The outer regions appear diffuse and somewhat irregular, lacking well-defined spiral arms or disk structures. There is a hint of minor asymmetry, potentially suggesting a past interaction or minor disturbance, but no prominent signs of ongoing mergers are visible. The overall appearance points towards a relatively evolved galaxy, likely with a significant population of older stars.
