The galaxy presents as a centrally concentrated system with a smooth, featureless morphology. It has an elliptical shape, elongated along a major axis. The central region appears brighter and exhibits a yellowish-orange hue, possibly indicative of an older stellar population. There's a color gradient moving outward from the center. The outer regions of the galaxy display a fainter, slightly bluer coloration, which may suggest the presence of younger, hotter stars, though star formation activity seems low overall. No distinct spiral arms or bar structures are visible. There is no visual evidence of any major mergers or tidal disturbances. The galaxy appears relatively isolated and undisturbed.
