This galaxy presents as a roughly elliptical or spheroidal system, appearing largely smooth in texture with a concentrated central bulge that emits strongly in visible light, indicating a substantial population of older stars. Faint tidal tails are visible extending from the galaxy's main body, potentially signifying a past or ongoing interaction or merger event. The tidal features are more blue, indicating that these structures contain younger stars. There is some evidence of internal structure, such as possible faint spiral arms or dust lanes, though the resolution limits certainty. The galaxy's color is predominantly yellow-red, implying a relatively low rate of current star formation.