The galaxy presents a generally elliptical morphology, with a high degree of central light concentration. The core region exhibits a bright, nearly unresolved appearance, possibly indicative of an active galactic nucleus or a dense stellar population. The overall color profile suggests a relatively evolved stellar population, with a redder hue dominating the central and outer regions. However, faint blue patches or subtle extensions are present on one side, potentially indicating regions of more recent star formation. No pronounced spiral arms or bar structures are evident. The galaxy displays a subtle disk like asymmetry. There is no obvious evidence of a major merger event, although there might be minor disturbances, possibly from a past interaction with a smaller object. A large fraction of the light appears to be uniformly distributed, and there is some indication of disk morphology.
