This galaxy presents as a relatively smooth, centrally concentrated object. The primary light appears yellowish-white, suggesting a population of older stars. The shape is elliptical, tending towards round but not perfectly so. There is little evidence of spiral arms or significant dust lanes. No obvious signs of a major merger or significant tidal disturbances are visible. The galaxy has a distinct core with luminosity that fades smoothly towards the edges, indicating a relaxed stellar population.
