The galaxy presents as a single, relatively smooth object. There is a bright, concentrated central region, possibly indicative of a galactic bulge. The light appears to be radially symmetric, with a diffuse outer region that gradually fades into the background. The galaxy appears to have an elliptical morphology; there is little to no evidence of spiral arms or a distinct disk structure. The color profile suggests a mature stellar population, appearing more reddish or yellowish than blue. There is no clear indication of a recent merger event or significant tidal disturbances based on the absence of extended tails or asymmetrical features.
