The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. Its core emits strongly, suggesting a high concentration of older stars. The overall color profile is yellowish-red, indicative of a population dominated by older, redder stars, implying low levels of ongoing star formation. There is little evidence of spiral arm structure or dust lanes. There is a hint of some mild disturbances in the galaxy, possibly from a past or ongoing merger event. The light profile is relatively smooth with hints of a slight elongation.
