The galaxy presents a smooth, elliptical morphology. There is a bright central bulge that dominates the galaxy's luminosity profile. The galaxy's overall shape is elongated, and the light distribution appears relatively even, with no discernible spiral arm structure or prominent dust lanes. The color gradient suggests a population of older stars, concentrated towards the central region. The outer regions display a slightly bluer hue, hinting at the presence of younger stars, although this component is not visually dominant. The orientation suggests that the galaxy is observed at a moderate inclination angle. There is a small hint of a disk structure but not enough to classify it beyond the morphology of an elliptical galaxy.
