The galaxy presents as a relatively smooth, elliptical-like structure. The object appears largely featureless with no apparent spiral arms, dust lanes, or distinct morphological sub-structures. A uniform, yellowish-orange hue dominates the galaxy's composition, indicative of an older stellar population. The galaxy exhibits a high degree of central concentration. It displays a nearly circular appearance, with a hint of elongation. There are no signs of significant tidal disturbances or ongoing major merging events. A slight asymmetry may be present in the outer isophotes, but it's not conclusive.
