The galaxy presents as a generally smooth, somewhat rounded structure. It exhibits a concentration of light towards the center, suggesting a prominent galactic nucleus. The overall color appears to be a pale blue-white, potentially indicating a population of relatively young, hot stars. There's a subtle hint of a surrounding disk, though it is not sharply defined, with faint, diffuse extensions outwards. There is some indication of minor disturbances in the morphology, such as slight asymmetries in the outer regions, which might suggest past or ongoing interactions with other galaxies. Overall, the galaxy presents an intermediate luminosity and moderate star forming rate.
