The galaxy presents as a centrally concentrated object, exhibiting a smooth, elliptical morphology. A bright, relatively uniform core is visible, surrounded by a more diffuse halo. Color gradients suggest older stellar populations dominate, with the central region exhibiting a yellow-white hue, potentially indicative of evolved stars. There is no obvious spiral structure. The overall round appearance suggests it is likely an elliptical galaxy viewed from a near face-on perspective. There is no evidence of significant tidal disturbances or ongoing mergers based on visual inspection.
