The galaxy presents a predominantly smooth, elliptical morphology. The light distribution appears centrally concentrated, lacking prominent spiral arms or a distinct disk. There is a slight elongation of the galactic body, with an estimated axis ratio of approximately 9:10 (ba50/90). The galaxy exhibits a color gradient, with the central region appearing bluer compared to the surrounding halo, which displays a redder hue. This suggests a possible difference in stellar populations, where the core may contain younger, hotter stars compared to the outer regions. There is no obvious sign of tidal disturbances or ongoing major merging events, yet there is a slight disturbance on one side of the galaxy indicating a possible past minor disturbance. Overall, the galaxy appears relatively undisturbed and evolved, likely undergoing a low rate of star formation.
