The galaxy presents as an elliptical morphology. It displays a smooth, concentrated central bulge with a gradual decrease in luminosity outwards, lacking distinct spiral arm structures. The color profile suggests an older stellar population, with a yellowish-orange hue indicating a paucity of recent star formation. There is a slight asymmetry to the galaxy's shape, potentially indicative of a minor gravitational interaction or past merger event. The light distribution suggests the galaxy is relatively round in shape, rather than elongated or cigar-shaped. There are no clear signs of a major ongoing merger or significant tidal disturbances. Overall, the galaxy appears to be a relatively quiescent system with a large mass and very low star formation rate.
