The galaxy presents as an elliptical morphology, with a smooth, spheroidal light distribution and minimal discernible features. Its color profile suggests a dominant population of older stars, as the central region exhibits a yellow-white hue, indicative of lower star formation rates. A faint halo of redder light surrounds the central core, possibly due to the presence of a population of cooler, older stars extending outwards from the galaxy's main body. There is no obvious evidence of spiral arms, bar structures, or significant dust lanes. The galaxy appears relatively undisturbed, with no signs of ongoing major mergers or tidal interactions. Its overall appearance suggests a mature, quiescent system.
