The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge region with a yellowish hue, suggesting an older stellar population. The main body of the galaxy appears generally rounded, with a slight elongation. Faint, diffuse extensions or tidal features are tentatively observed, possibly indicative of minor gravitational interactions or past merger events. Overall, the galaxy appears relatively undisturbed with no prominent spiral arm structures readily discernible. Star formation is likely present, but at a modest rate.
