The galaxy presents as a relatively bright, elliptical-like object, exhibiting a smooth, featureless morphology. Color gradients are subtle, transitioning from a yellowish core to slightly redder outer regions. The overall form suggests an oblate spheroid shape. There is no evidence of spiral arms, bars, or significant dust lanes. The light distribution is concentrated towards the center, with a diffuse halo extending outwards. Based on the concentration of light, this is likely an older stellar population. There is no evidence of ongoing major mergers or tidal disturbances.
