The galaxy presents with a moderately elliptical morphology, appearing somewhat elongated rather than perfectly spherical. Its central region exhibits a concentrated luminosity, suggesting a prominent galactic nucleus. The color gradient indicates a population of older stars, with a redder hue dominating the central bulge and a gradual shift toward slightly bluer tones in the outer regions. Faint, disturbed features are visible in the outer disk, hinting at possible gravitational interactions or past minor mergers. Overall, the galaxy appears relatively smooth, though it is not perfectly uniform with these slight disturbances.
