The galaxy presents a morphology that is somewhat disturbed, likely due to interactions or internal processes. The primary body of the galaxy exhibits a relatively smooth light distribution, suggestive of an elliptical galaxy or a spiral galaxy viewed at a high inclination. The central region displays a strong concentration of light, indicating a prominent galactic nucleus or bulge. A noticeable elongation is present, deviating slightly from a perfectly spherical shape. The color profile exhibits variations, with a central yellowish-white hue, indicative of older stellar populations, and a slightly bluer and fainter glow extending outward. There also seems to be a disturbance, possibly a smaller galaxy or a knot of star formation, located close to the galaxy.
