The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that appears yellowish, indicating an older stellar population. The galaxy's overall shape is elongated, with an intermediate ellipticity, neither perfectly round nor highly elongated. Faint, diffuse outer regions are visible, extending beyond the brighter central area, suggesting a gradual decline in stellar density. There's a subtle indication of a minor disturbance in the morphology, but no clear signs of a recent major merger or significant tidal disruption. The galaxy’s redshift suggests that it is a distant object. The galaxy's apparent color is redder than expected, possibly due to its redshift and the presence of older stars.
