The galaxy presents as a relatively smooth, elliptical morphology. The light profile appears centrally concentrated with a gradual decrease in intensity outwards, showing a diffuse halo. The galaxy exhibits a yellowish-white hue, suggesting a stellar population dominated by older, evolved stars. There is little evidence of distinct spiral arms, dust lanes, or active star formation regions. The overall structure appears undisturbed, without significant tidal features or signs of ongoing mergers. The galaxy displays a nearly circular shape.
