The galaxy presents a generally smooth, elliptical morphology. Its central region exhibits a bright, concentrated core that appears almost spheroidal. Surrounding this core is a more diffuse halo of light, suggesting a gradual decrease in stellar density with increasing distance from the center. There may be a hint of minor structural asymmetry, with a slight elongation or tidal feature extending from one side of the galaxy, possibly indicative of a past or ongoing interaction. The overall color is yellowish, implying a population of older stars and a relatively low rate of current star formation. There are several slightly brighter spots or knots of material within the galaxy, perhaps star clusters, but overall there is no evidence of spiral arm structure or significant dust lanes.
