This galaxy presents a generally smooth, elliptical morphology. The light is centrally concentrated, displaying a bright, yellowish core that gradually diffuses outwards. There is minimal evidence of spiral arm structure or significant dust lanes within the visible light. The object exhibits a moderately round shape, deviating slightly from a perfect circle. The color gradient suggests the presence of an older stellar population, potentially indicating a lower rate of star formation. There is no clear indication of a major ongoing merger event, although subtle irregularities in the outer regions could potentially hint at minor gravitational interactions. The overall appearance suggests a galaxy that is relatively evolved, with a high degree of symmetry and a relatively passive star formation history.
