The galaxy presents as a single, centrally concentrated object with a smooth, diffuse light distribution. It appears roughly circular in shape, exhibiting a high degree of symmetry. The central region shows a concentration of light, decreasing in intensity outwards in all directions. The galaxy exhibits a color gradient, transitioning from a yellowish central region to a redder halo. No distinct spiral arms or prominent dust lanes are discernible. The overall appearance suggests a relatively evolved system with a well-mixed stellar population. There is no evidence of ongoing major mergers or significant tidal disturbances. The red color indicates the presence of older stars.
