The galaxy presents an elliptical morphology, exhibiting a smooth, centrally concentrated light distribution. Its color profile reveals a predominantly yellowish-orange hue in the central region, possibly indicating an older stellar population. Fainter, bluer outskirts suggest the presence of some younger stars, though these regions are not prominent. The overall structure appears relatively undisturbed, with no obvious signs of ongoing major mergers or tidal interactions. There is a slight deviation from perfect circularity, trending towards an intermediate ellipticity.
