The galaxy appears to be an elliptical galaxy, characterized by its smooth, relatively featureless morphology. It exhibits a slightly elongated shape, appearing more in-between round and cigar-shaped than either extreme. There is no discernible spiral structure or prominent disk. The galaxy's light profile appears centrally concentrated with a gradual decrease in brightness outward from the core. No major or minor disturbances are observed, suggesting the galaxy is not currently undergoing a significant merger event. The overall color appears to be towards the redder end of the spectrum, potentially indicating an older stellar population with lower rates of ongoing star formation.
