The galaxy presents as a somewhat elliptical structure, exhibiting a smooth morphology with no obvious spiral arms or bar. The central region displays a concentrated, bright core that appears to be spheroidal in shape. A gradual decrease in luminosity is observed from the core outwards, forming an extended halo. There is some slight evidence of a disk component in the outer regions with a faint, diffuse, greenish hue. The major axis of the galaxy is clearly longer than the minor axis indicating an elliptical shape rather than being perfectly circular. There is no indication of any significant mergers or tidal disturbances. The galaxy's overall color index suggests a population of older stars. There is some indication of ongoing star formation, evidenced by faint bluer regions surrounding the central bulge.
