The galaxy presents a slightly elongated, irregular morphology. A bright, concentrated central region dominates, exhibiting a cyan-blue hue. This suggests active star formation or a significant population of hot, young stars. Fainter, reddish-purple patches surround the central region, possibly indicating areas of dust obscuration or older stellar populations. Faint wisps or tails appear to extend from the main body of the galaxy, hinting at possible gravitational interactions or recent merger events. The galaxy exhibits notable features and a lack of a smooth, elliptical structure.
