The galaxy presents as a relatively smooth, elliptical structure. There is a concentrated central bulge exhibiting a yellowish-white hue, suggesting a population of older stars. The surrounding disk, though not sharply defined, appears elongated and cigar shaped. The overall color gradient from the center outwards suggests a gradual decrease in stellar density and possibly an increase in younger stellar populations within the outer regions of the galaxy. There are no obvious signs of major merging events or strong tidal disturbances.
