The galaxy presents as a somewhat elliptical, centrally concentrated object. The core appears a yellow-white hue, suggesting an older stellar population. The outer regions display a fainter, more diffuse structure, potentially indicating the presence of a stellar halo. No distinct spiral arms are visible, and the overall morphology appears relatively smooth, with no strong evidence of major disturbances or ongoing mergers. There is the slightest hint of blue in the upper region, hinting at some star formation. The galaxy appears to be in a relatively evolved state.
