The galaxy appears as an elliptical-like structure, exhibiting a high degree of radial symmetry. The light profile suggests a smooth distribution, with no apparent spiral arms or prominent disk features. The central region presents a bright, concentrated core that gradually fades towards the outer edges. Color gradients are subtle, but the core exhibits a slightly yellow-shifted hue, transitioning to a redder color in the outer regions, indicative of an older stellar population. There is no visual evidence of ongoing mergers or significant tidal disturbances. The overall morphology suggests a galaxy dominated by an evolved stellar population with a relatively low rate of star formation.
