The galaxy presents a generally smooth, elliptical morphology. There is a bright, concentrated central bulge that dominates the galaxy's luminosity. A faint, diffuse halo surrounds the central bulge, extending outwards. The galaxy appears slightly elongated rather than perfectly spherical. There is a hint of a disk-like structure, but it is not well-defined, suggesting it is viewed at an angle or that the disk is relatively small. The overall color is yellowish-white, indicating a population of older stars. There may be some minor gravitational disturbance or interaction occurring with a small distortion visible on one side of the halo. No significant dust lanes or spiral arm structures are discernible. Overall, it appears to be a relatively massive galaxy with a moderate rate of star formation.
