The galaxy presents as a relatively smooth, elliptical structure, with a high degree of circularity. Its light profile is centrally concentrated, displaying a bright core that graduates outward to a fainter, diffuse halo. The color indices suggest a population of older stars dominating the light output, giving the galaxy an overall reddish-yellow hue. There is no obvious evidence of significant spiral arm structure or prominent dust lanes. Faint extensions may be present but are not well defined, showing very minor disturbances. The galaxy appears to be in a relatively quiescent state, with indications of low star formation activity.
