The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a centrally concentrated light profile, suggesting a prominent bulge component. The overall color appears to be somewhat redder, indicative of an older stellar population and lower star formation activity. There is little evidence of spiral arms or a distinct disk structure. The galaxy appears to be isolated, with no obvious signs of major mergers or tidal disturbances in its immediate vicinity, though minor interactions cannot be ruled out. The shape is nearly circular, suggesting it is viewed close to face-on.
