The galaxy presents a complex morphology, exhibiting features suggestive of both smooth and disturbed structures. A concentrated central region dominates the galaxy's light profile, appearing relatively smooth and bright, possibly indicating a bulge component. However, the surrounding regions show signs of irregularities, potentially indicative of tidal interactions or ongoing mergers. Faint extensions or distorted arms are visible, hinting at gravitational disturbances. The color distribution within the galaxy is varied, with a blueish hue in the central regions and a shift towards redder tones in the outer parts, potentially reflecting differences in stellar populations or dust content across the galaxy. Overall, this galaxy's morphology suggests a dynamic system undergoing interactions or exhibiting recent merger activity.
