The galaxy presents as a relatively smooth, centrally concentrated object with a high degree of circular symmetry. The light distribution appears to be dominated by a central bulge component with a gradual decline in surface brightness outward. Faint blue-green emissions surround the central bulge. No obvious spiral arm structures or dust lanes are discernible. It appears to be relatively isolated, showing no signs of major interaction with neighboring galaxies in this field of view. This galaxy would classify as an early-type galaxy based on morphology. The estimated size is relatively small, around 2 kpc.
