The galaxy presents a predominantly smooth, elliptical morphology. It appears as a diffuse, centrally concentrated object with a gradual decrease in luminosity outwards. There is a slight elongation, suggesting it is not perfectly spherical, but rather leans towards a cigar shape. No distinct spiral arms or prominent dust lanes are discernible. The color profile suggests a higher concentration of older stellar populations, indicated by its reddish hue. There are no obvious signs of major ongoing mergers or significant tidal disturbances in its immediate vicinity, though a minor disturbance cannot be ruled out due to the fuzziness of the image.
