The galaxy presents as a smooth, centrally concentrated object. It exhibits an elliptical morphology with a slight elongation, appearing somewhere in between round and cigar-shaped. The galaxy’s light is dominated by a yellowish-white hue, suggesting a stellar population that is somewhat evolved. A redder tinge is observed in a region of the galaxy, possibly indicative of older stellar populations or dust obscuration in that area. The overall structure seems largely undisturbed, without any prominent signs of ongoing mergers or significant tidal disruptions. The absence of clearly defined spiral arms or significant disk-like structures suggests this galaxy may be classified as an elliptical or lenticular galaxy.
