The galaxy presents as a roughly elliptical, moderately compact structure. The core region exhibits a bright, relatively concentrated luminosity, suggesting a high stellar density in the galactic nucleus. There's a fairly smooth, gradual fall-off in luminosity from the center to the outer regions, with no distinct spiral arm features immediately apparent. The color profile indicates a slightly bluer hue, particularly in the core, hinting at ongoing star formation processes. A slight disturbance to the primary mass distribution seems to be present, with a lopsided appearance of mass. The general morphology is more closely aligned with an early-type galaxy such as an elliptical or lenticular galaxy.