The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a round morphology, with a very slight elongation. The core region displays a yellowish hue, suggesting a population of older stars. The outer regions show a subtle decrease in intensity and shift toward a bluer color, potentially indicating some younger star formation. No distinct spiral arms or prominent dust lanes are discernible in this image. There are no obvious signs of significant tidal disturbances or ongoing mergers, although the possibility of a minor past interaction cannot be entirely ruled out. Overall, the galaxy appears to be a relatively evolved system.
