The galaxy presents an elliptical morphology, appearing largely smooth and centrally concentrated. It exhibits a radial color gradient, transitioning from a warm yellowish-orange core to cooler greenish outer regions. The central bulge is well-defined and dominates the galaxy's overall luminosity. Faint, asymmetric extensions are discernible, possibly indicative of minor gravitational interactions or past merger events. While a disk component is not readily apparent, subtle irregularities in the outer regions could suggest faint spiral arms or tidal features. There is no singular, prominent structure in the galaxy. The overall structure suggests a mature system undergoing star formation.
