The galaxy presents as a generally smooth, elliptical-like structure. There is a concentrated central bulge that is bright and yellowish in color, indicating an older stellar population. The galaxy lacks discernible spiral arms or a prominent disk. It exhibits a high degree of roundness. There are no indications of significant ongoing mergers or tidal disturbances in its immediate vicinity. The galaxy appears relatively isolated and unperturbed. Based on its color and morphology, the galaxy is consistent with being an early-type galaxy with a relatively low star formation rate.
