The galaxy presents as a generally smooth, elliptical object with a slight central concentration of light. There is minimal evidence of spiral arms or other significant disk-like features. The color profile appears relatively uniform across the galaxy, with a slight reddening towards the center and a subtle blueish hue in the outer regions. The overall round appearance and smoothness indicate a likely classification as an elliptical galaxy, possibly of type E3-E5 on the Hubble sequence. There are no obvious signs of ongoing major mergers or significant tidal disturbances, though subtle minor disturbances cannot be ruled out. The galaxy is moderately luminous, suggesting a substantial stellar population and total mass.
