The galaxy presents as a somewhat elliptical, centrally concentrated light distribution. The core region exhibits a high degree of smoothness and a yellow hue. The outer regions display a more diffuse and fainter light distribution, with a subtle transition in color towards a bluer shade compared to the core. Evident of some minor morphological disturbances or features beyond the core. The galaxy appears relatively isolated in this field of view, showing no clear signs of on-going major merger activity, although some minor interaction cannot be ruled out based on observed faint features. Based on the overall morphology, the galaxy is most likely an elliptical or lenticular type.
