The galaxy presents as a singular, concentrated object with a generally smooth morphology. The light profile appears relatively symmetrical and centrally concentrated, displaying a slightly elliptical form. Its overall color leans towards the red end of the spectrum, suggesting a population of older stars or significant dust obscuration. There is a subtle hint of a diffuse, extended halo surrounding the central region, though it blends smoothly into the background. No distinct spiral arms or features of ongoing major mergers are discernible. The structure appears largely undisturbed, showing no significant tidal tails or other signs of recent disruptive interactions.
