The galaxy presents as a fairly smooth, centrally concentrated object. Its overall shape appears largely elliptical, with a high degree of circularity. There is a subtle color gradient, with a slightly bluer hue concentrated towards the galactic center, suggesting the presence of younger, hotter stars in that region, potentially indicative of recent or ongoing star formation. The outer regions display a redder hue, possibly due to an older stellar population. The galaxy appears relatively undisturbed, lacking any obvious signs of major mergers or tidal interactions. There are no clear spiral arm structures or a prominent disk visible. A very faint hint of extended emission may be present, but is difficult to ascertain from the data provided. Overall, the galaxy seems to be a relatively quiescent system.
