The galaxy presents as a smooth, centrally concentrated object, displaying an elliptical morphology. There is an apparent lack of spiral arm structures or significant dust lanes. The central region is bright, with a yellow-red hue, possibly indicative of an older stellar population. The light intensity gradually decreases from the core outwards, showing a relatively diffuse outer halo with a slight elongation along its major axis. There is no visual evidence of any ongoing major merging events or significant tidal disturbances. The galaxy appears relatively isolated and undisturbed.
