The galaxy presents a predominantly elliptical morphology, elongated along its major axis. The light profile appears smooth and centrally concentrated. The color gradient suggests a relatively homogeneous stellar population, with a slight reddening towards the core, consistent with an aging stellar population. There is no clear indication of spiral arm structure or significant dust lanes, but a slight asymmetry is noticeable in its overall shape. The galaxy's overall appearance is consistent with a relatively evolved system undergoing passive evolution, with little active star formation.
