The galaxy presents as a largely smooth, elliptical morphology. There is little evidence of spiral arm structure or prominent dust lanes. The light profile appears centrally concentrated, with a gradual falloff in surface brightness from the core to the outer regions. The color is generally yellowish, suggesting a population of older stars. Slight bluer hues are present, suggesting there is some ongoing star formation, albeit at a low rate. There is no visible evidence of a major ongoing merger or tidal disturbance affecting the overall structure. The galaxy presents a primarily rounded shape.
