The galaxy presents as a luminous, centrally concentrated object. It appears to be primarily smooth in texture with a largely elliptical morphology, approaching a circular form. The core region exhibits a yellow-orange hue, suggesting a population of older stars. The outer regions show a slight blue tinge, which hints at the presence of a younger stellar population, but the galaxy is dominated by its redder, older population. There are no clear signs of strong spiral arm structures or bar features. Subtle irregularities are present, indicating minor disturbances. Overall, it appears as a well-formed system, likely relatively quiescent in terms of active star formation. The galaxy appears to be in a relatively isolated state, without nearby interacting companions.
