The galaxy presents a largely smooth morphology. It exhibits a centrally concentrated light distribution that gradually decreases with radial distance. The overall shape appears nearly circular in projection, lacking any obvious disk-like structures or spiral arms. The core of the galaxy is characterized by a bright, yellowish color, suggesting a population of older stars. There is a subtle color gradient as one moves outwards from the core to the outer regions; it appears slightly bluer, hinting at the possibility of some low-level star formation activity, though the rate is likely quite low. No significant signs of tidal disturbances, mergers, or interactions are detected.
