The galaxy appears as a centrally concentrated object with a relatively smooth, elliptical morphology. There is a slight elongation, but it generally presents as quite round in form. The galaxy exhibits a color gradient, with a whiter, possibly bluer core region, suggesting some level of recent star formation, and redder outskirts indicating a somewhat older stellar population is dominant in the outer regions. There is no clear evidence of significant spiral structure or strong tidal disturbances. Faint signs of a disk-like component may be present, but are not obvious. Any ongoing merger activity appears unlikely. Overall, the galaxy shows characteristics consistent with an early-type galaxy, possibly undergoing some recent star formation.
