The galaxy appears to be a relatively smooth, elliptical-like structure. There is a high degree of central concentration, with the light intensity peaking towards the core. The light is more yellow in the center and has a blue glow surrounding it. The galaxy appears relatively isolated, with no obvious signs of major tidal disruption or ongoing mergers. It is likely that there has been some form of minor disturbance based on the subtle asymmetry in the shape and halo around the light source. There is no indication of strong dust lanes or prominent spiral arm structures in this imaging.
