The galaxy presents as a relatively smooth, centrally concentrated object. The light profile appears roughly elliptical, with a slight deviation from perfect circularity; exhibiting a round shape. A color gradient is visible within the galaxy, with a reddish hue concentrated towards the core and a bluer tint in the outer regions. No distinct spiral arm structures or prominent dust lanes are discernible. The overall morphology suggests a relatively evolved system, possibly an elliptical galaxy or a lenticular galaxy seen at a shallow inclination. There is some evidence of a minor disturbance present in the form of faint asymmetry, suggesting the possibility of past interactions.
