The galaxy presents as a moderately bright, elliptical structure. The light distribution appears relatively smooth and centrally concentrated, with a diffuse halo extending outwards. Color gradients suggest an older stellar population, with a yellowish-orange hue dominating the central regions, potentially indicating the presence of evolved stars. There is some evidence of bluer light in the outer disk, potentially indicating some star formation. There are no distinct spiral arms or a prominent bar. The overall morphology suggests this could be an early-type galaxy, possibly an elliptical or lenticular galaxy seen at an angle. The lack of significant morphological disturbances points to a relatively undisturbed evolutionary history, with no apparent major merger events.
