The galaxy presents as a smooth, elliptical-like structure, displaying a concentrated central bulge that emits a significant amount of yellow light. There is a less luminous halo surrounding the central bulge. The overall color profile suggests a population of older stars dominating the galaxy's stellar content, implying a relatively low rate of current star formation. The shape is primarily oblong with a slight degree of asymmetry. There are no apparent signs of ongoing major mergers or tidal disturbances, though a minor interaction cannot be entirely ruled out. 
