The galaxy appears to be a relatively smooth, elliptical structure. It presents with a central bulge that appears concentrated and gradually fades into an extended halo. There are no clear spiral arms or bar structures visible. The overall color of the galaxy suggests a higher proportion of older stars. The galaxy displays an approximately intermediate axial ratio, appearing neither perfectly circular nor highly elongated. There is a hint of minor asymmetry or a slight disturbance in the outer regions of the halo, potentially indicating a past minor merger or tidal interaction. No signs of major mergers or significant tidal disruptions are observed.
