The galaxy presents a roughly elliptical morphology, exhibiting a relatively smooth appearance with some irregularities. It appears diffuse, lacking a clearly defined nucleus. Color gradients suggest a redder core region transitioning to a slightly bluer outer halo. There is a subtle indication of possible tidal features or minor disturbances in the outer regions. A secondary point source of light is visible nearby, which is likely the cause of the observed disturbance. No distinct spiral arms or bar structures are readily apparent. 
