The galaxy presents a somewhat elliptical morphology, though not perfectly spherical. It appears relatively smooth in texture. The central region exhibits a concentrated luminosity, suggestive of a prominent galactic bulge. Moving outward from the center, the intensity of light gradually diminishes. There's a faint indication of a possible disk-like structure, but this is not clearly defined. Slight asymmetrical features suggest potential tidal disturbances and perhaps a minor merger. The overall coloration indicates a population of older stars.
