The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The light distribution suggests a higher density of older stars in the core, which appears yellowish. Moving outwards from the center, the galactic halo exhibits a bluer hue, possibly indicating a population of younger stars. The overall shape is elongated, but not extremely cigar-shaped, indicating a slight degree of ellipticity. Some minor disturbances or asymmetries are faintly visible, primarily as slight irregularities in the outer regions, suggesting possible past gravitational interactions or minor mergers. There is a subtle hint of a disk-like structure, but it is not clearly defined, and the galaxy appears to be primarily bulge-dominated.
