This galaxy presents as a largely homogenous, rounded object. The core exhibits a bright, concentrated luminosity with a slight bluish-white hue, suggesting a population of relatively young, hot stars or an active galactic nucleus. There is a gradual decrease in surface brightness moving outward from the center. The outer regions of the galaxy display a faint, diffuse halo with a subtle reddish tint. The overall smooth appearance and lack of prominent features such as spiral arms or a distinct bar structure indicates it is most likely an elliptical or lenticular galaxy. There is no indication of any major ongoing merging activity or significant tidal disturbances.