The galaxy presents as a relatively smooth, elliptical-like structure, appearing more elongated than circular. The central region displays a brighter, more concentrated luminosity, indicative of a dense galactic nucleus. Moving outwards from the center, the intensity of light gradually diminishes, blending into the surrounding background sky. There is a slight suggestion of a disk-like component. Evidenced from color variations it is likely comprised of a dominant population of older stars, although some active star formation may be occurring, given the bluer hues observed. No obvious signs of major mergers or significant tidal disturbances are immediately apparent, yet the slight asymmetry cannot rule out prior minor gravitational interactions. The galaxy presents a well-defined structure with a notable central bulge and gradual decline in stellar density towards its periphery. 
