The galaxy presents as a roughly elliptical structure with a dominant, smooth light profile. The central region exhibits a higher concentration of light, transitioning to a more diffuse outer halo. There is an indication of bluer light in the central region of the galaxy, with the outer regions appearing slightly redder in comparison. This difference in color suggests that the stellar populations might be slightly different between these regions. There is the possibility of minor disturbances, but the overall structure is well-defined. The galaxy is not perfectly round and is somewhere in between round and cigar shaped. 
