The galaxy appears to be largely smooth and elliptical in shape, with a generally round morphology. The primary body of the galaxy exhibits a relatively uniform surface brightness, indicating a lack of strong spiral arm features or significant dust lane obscuration. There is evidence of a possible minor disturbance in the galaxy's structure. A secondary, smaller object appears nearby and may be gravitationally interacting with the primary galaxy, inducing tidal forces. The apparent blueness of the galaxy's light indicates a population of younger, hotter stars, or potentially, significant star formation activity occurring within the galaxy. The light intensity appears to decrease gradually from the center of the galaxy to its outer edges. 
