The galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated light distribution. There is a distinct lack of resolved spiral arm structures or prominent dust lanes. The galaxy's shape is generally spheroidal, verging on slightly elongated, with a fairly high degree of central concentration. It presents a gradual decrease in luminosity outwards from its core, which contains a yellowish hue and possibly older stars. The extended halo has a bluish color. There is no evidence of significant tidal disturbances, major mergers, or ongoing star formation. The galaxy displays a notable red color, indicating a potentially older stellar population and a low star formation rate.
