The galaxy presents a smooth, centrally concentrated morphology, lacking any prominent spiral arms or bar structures. Its overall shape appears nearly circular. The light profile suggests a single component system, with a gradual decrease in intensity from the core outwards. There is no clear evidence of ongoing major mergers or significant tidal disturbances. The galaxy's color indices indicate a population of evolved stars, consistent with a relatively passive star-formation history. There is a slight asymmetry to the morphology that could indicate a minor disturbance from a past interaction, but that is not definitive. The angular size appears compact, suggesting the galaxy is at a considerable distance.
