The galaxy presents a primarily smooth morphology, with a slight elongation in its overall shape. The color profile suggests a relatively old stellar population, as indicated by the reddish-yellow hue, implying lower rates of on-going star formation. There is no obvious presence of spiral arms or a distinct disk structure. Faint hints of disturbances in the outer regions are present, but there is no significant evidence of an active ongoing merger with another galaxy, or any major tidal distortions. The central region appears brighter and more concentrated than the outer regions, typical of an elliptical or lenticular galaxy. Overall, the galaxy appears as a relatively undisturbed, evolved system.
