The galaxy appears as a single, largely featureless object. It exhibits a concentrated central bulge that decreases in luminosity with radial distance. The galaxy's morphology is generally smooth and elliptical, with a high degree of roundness. There's no evidence of spiral arms or a significant disk structure. Based on its color profile, the galaxy's stellar population appears dominated by older, redder stars. There does not seem to be any evidence of ongoing mergers or disturbances in the galaxy's structure, such as tidal tails or asymmetrical features. Overall, this galaxy seems to be an elliptical galaxy that has completed the major star forming phase of its lifetime.
