The galaxy presents as a relatively smooth, centrally concentrated object with a noticeable red hue. There is no clear evidence of spiral arms or a distinct disk. The light distribution appears fairly uniform across the galaxy, with a gradual decline in intensity moving outwards from the center. The shape is somewhat elliptical. There is a slight indication of minor disturbances, such as asymmetry in its form. Overall, the galaxy exhibits characteristics consistent with an elliptical or lenticular morphology, with a relatively high degree of smoothness.
