The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The core region displays a prominent yellowish hue, indicative of an older stellar population and reduced ongoing star formation activity. Moving outwards from the core, a gradual decrease in surface brightness is observed. The outer regions exhibit a faint, blue-ish tinge. This may suggest a sparse population of younger, hotter stars, though it's more likely residual effects from background light. The galaxy appears largely undisturbed with no obvious signs of recent or ongoing major mergers or significant tidal interactions. The overall shape is not perfectly spherical, exhibiting a slight elongation, more closely resembling a lenticular or elliptical galaxy type than a spiral. The galaxy possesses significant mass. However, the rate of new star formation within the galaxy is relatively low.
