The galaxy presents a generally smooth morphology, appearing elliptical in shape. It exhibits a concentration of luminosity towards the central region, with a gradual decrease in surface brightness moving outwards. There is little evidence of spiral arm structure or significant dust lanes. The color profile suggests a possible presence of older stellar populations, particularly within the core. There is no immediately apparent indication of a major ongoing merger event. However, a minor disturbance cannot be ruled out due to the slight asymmetry in the outer regions of the galaxy. The overall impression is that of a relatively evolved system, possibly an early-type galaxy or a bulge-dominated spiral observed at a significant redshift.
