The galaxy presents as a relatively smooth, centrally concentrated object. It appears elliptical in shape, exhibiting a high degree of symmetry. There is a slight elongation observed, but it is close to a circular morphology. The light distribution is centrally peaked, with a gradual falloff in intensity towards the outer regions. Color gradients are subtle; however, the central region appears slightly bluer than the more diffuse outer regions. This suggests the presence of a younger stellar population in the core relative to the galactic halo. No distinct spiral arms or prominent dust lanes are visible, and the galaxy lacks any major disturbances. Faint traces of a very minor disturbance is possible, which is represented in the outer regions as a slight asymmetry in its light profile. Overall, the galaxy's appearance suggests a quiescent system.
