The galaxy appears as a relatively smooth, elliptical-like structure. Its core exhibits a concentrated, bright, yellowish-white hue, suggesting a population of older stars. There are faint suggestions of a disk structure surrounding the center of the galaxy, however, the disk is not well-defined. The outer regions of the galaxy fade in intensity and show a slightly reddish tint compared to the core, possibly indicating a difference in stellar populations, dust content, or a decrease in star formation activity in those regions. The overall form is generally round, with no obvious signs of major disturbances or ongoing mergers. The galaxy is relatively compact.