The galaxy appears to be a relatively compact system with a smooth, elliptical morphology. There is a brighter, yellowish core, surrounded by a more diffuse and somewhat bluer halo or disk-like structure. The overall shape is somewhat rounded. There might be minor tidal disturbances or a possible merger in progress due to the irregular outer regions and the existence of the disk. There is no clear spiral arm structure visible. The colors suggest a mix of stellar populations, with the central region possibly dominated by older, redder stars and the outer region having a greater proportion of younger, bluer stars and regions of active star formation.
