The galaxy presents as a single, largely featureless object with a smooth, elliptical morphology. The central region exhibits a concentrated, bright core, potentially indicative of a supermassive black hole or a dense stellar population. Progressing outward from the core, the light profile gradually diminishes, with no apparent spiral arms, bars, or distinct substructures.

Color gradients are subtle, suggesting an overall evolved stellar population. The central region appears somewhat more yellow-orange, possibly due to older, cooler stars. A faint blue halo surrounds the galaxy. No significant signs of ongoing major mergers or tidal disturbances are apparent in the immediate vicinity, although minor disturbances may be present. The overall impression is of a relatively quiescent, massive galaxy, likely an elliptical or S0 type.
