The galaxy presents a generally smooth and elliptical morphology. It appears quite round in shape. There is no apparent spiral structure or distinct disk component visible. The galaxy exhibits a centrally concentrated luminosity profile. A subtle color gradient is observed, with a slight reddening towards the galaxy's core, indicating a potentially older stellar population in the central regions. There is no strong evidence of any major merger events or significant tidal disturbances in this image, though the possibility of minor interactions cannot be ruled out. The galaxy appears to be fairly isolated, with no immediately apparent companion galaxies that are interacting with it.
