The galaxy presents as a centrally concentrated object with a relatively smooth overall morphology. There appears to be a slight elongation to its shape, deviating somewhat from perfectly circular. The central region exhibits a higher surface brightness, characterized by a yellow-white hue, suggesting a population of older stars. The outer regions of the galaxy appear fainter and more diffuse, with a subtle color gradient towards a redder tone, possibly indicating a lower density of star formation or a difference in stellar populations compared to the core. No prominent spiral arms or distinct dust lanes are discernible, which supports the classification as a relatively smooth system. There is no obvious evidence of major mergers or significant tidal disturbances in this image.
