The galaxy presents a predominantly smooth morphology. Its shape appears largely round, with a slight deviation towards an intermediate elliptical form. The galaxy exhibits a centrally concentrated light profile, with a gradual decrease in luminosity towards its outer regions. There is some evidence of possible minor disturbances in the galaxy's structure, suggesting potential interactions or internal dynamic processes. Faint extensions could indicate possible tidal tails or merger remnants. The colour profile shifts from bluer hues in the center to redder in its outer regions.
