The galaxy presents as a relatively smooth, elongated structure. Its core exhibits a concentrated brightness, appearing yellowish-white. The galaxy's light gradually diminishes towards its outer edges. While it leans towards being elliptical in shape, subtle deviations suggest a possible disk-like component, though no distinct spiral arms are discernible. The red hue hints at a population of older stars dominating. There are no visually apparent signs of ongoing major mergers or significant tidal disturbances. The overall impression is that of a galaxy that is evolving slowly.
