The galaxy appears as a centrally concentrated object with a diffuse, somewhat elliptical halo extending outwards. The core exhibits a warmer, orange-tinted hue, suggesting an older stellar population or significant dust obscuration. The outer regions of the galaxy display a slightly bluer coloration, potentially indicating the presence of younger stars. No distinct spiral arms or bar structures are readily discernible. The galaxy appears relatively undisturbed, with no strong evidence of recent major mergers or tidal interactions. Overall, it presents as a relatively smooth, evolved system.
