The galaxy presents as a somewhat elliptical, centrally concentrated object. The core region exhibits a yellowish-white hue, suggesting a population of older stars. Surrounding the core, there's a broader, more diffuse halo with tinges of blue and green, hinting at the presence of younger stellar populations and possibly some ongoing star formation. The outer edges are indistinct, fading gradually into the background sky. There is no strong evidence of spiral arm structure, or of significant morphological disturbance. The galaxy appears relatively isolated and undisturbed. Overall, it has characteristics of a mature galaxy, likely an elliptical or lenticular type.
