The galaxy presents as a largely featureless elliptical type. It exhibits a concentrated central bulge with decreasing luminosity towards the outer regions. The overall shape appears mostly round, with a slight deviation toward an intermediate ellipticity. The galaxy's color suggests a stellar population dominated by older, redder stars. Evidence of recent or ongoing star formation appears to be minimal based on the lack of blue color. There is no visually apparent disk structure or spiral arm morphology. The galaxy seems undisturbed, with no signs of tidal interactions or major mergers. The lack of strong morphological distortions suggests it is a relatively isolated system or has undergone significant relaxation after any past interactions.