The galaxy presents as a somewhat amorphous, elliptical structure with a relatively smooth overall appearance. There is a concentration of light towards the central region, suggesting a galactic bulge or nucleus. The outer regions exhibit a more diffuse glow, fading gradually into the background. Faint hints of bluer tones are visible in the central areas, possibly indicating regions of younger star formation. There are no prominent spiral arms or other distinct features visible, leading to the determination of a fairly round, somewhat featureless galaxy with some degree of ongoing star formation. There is a very slight asymmetry, suggesting a possible minor gravitational interaction or previous merger event.
