The galaxy presents as a centrally concentrated object with a generally smooth morphology. It exhibits a slightly elliptical shape, appearing largely undisturbed with no obvious signs of major mergers or significant tidal features. The light profile suggests a dominant bulge component, with a color gradient indicating a population of older stars towards the galactic center and slightly bluer colors further out. There may be a very faint, diffuse disk component. No prominent spiral arms or dust lanes are discernible in the image. The galaxy appears to be a relatively passive system, with low star formation activity.
