The galaxy appears to be a relatively bright, elliptical object with a smooth light distribution. It exhibits a slight elongation, suggesting a deviation from a perfectly spherical shape. There is some indication of asymmetry in the outer regions. The core region presents a yellowish hue, potentially indicative of an older stellar population, while the fainter outer regions exhibit slightly bluer tints, which could point to younger stars or ongoing, though weak, star formation. Overall, the galaxy's morphology suggests a relatively evolved system, possibly in the process of merging.
