The galaxy presents an elliptical morphology, appearing as a somewhat flattened spheroid. Its core is characterized by a bright, concentrated luminosity, indicative of a high stellar density, likely an older stellar population. Proceeding outward from the core, the light gradually diminishes, with the outer regions appearing fainter and less structured. Hints of a faint disk are possibly present, though highly obscured by the overall smooth and elliptical nature. The galaxy exhibits a subtle color gradient from a yellowish white center to fainter, slightly bluer outer edges. No distinct spiral arm structures or prominent dust lanes are visible. Overall, the galaxy is a moderately large, early-type system with a smooth light distribution and an aged stellar population.
