The galaxy presents a generally smooth appearance with little discernible structure. It exhibits a moderately elliptical shape, transitioning from nearly round to somewhat elongated. There is no strong evidence of spiral arms or a central bar. There is no sign of a major merger or significant tidal disturbances. Color gradients suggest a potential redder core region transitioning to slightly bluer outer regions. This could indicate older stellar populations are more concentrated towards the center. Overall, this galaxy appears to be a relatively undisturbed system.
