The galaxy presents as a single, dominant, centrally concentrated object. It appears relatively smooth and elliptical in shape, with a high degree of central concentration. The galaxy exhibits a gradual decline in surface brightness from the core outward. There is no evidence of strong spiral arms, dust lanes, or significant star-forming regions visible in this image. The color appears generally yellowish, suggesting an older stellar population. The galaxy shows no obvious signs of major tidal disturbances or ongoing merging activity, although some minor irregularity in its outer regions cannot be ruled out. The galaxy is approximately 5.8 Kpc in radius. 
