The galaxy presents as an elongated, somewhat irregular structure. A central bulge region exhibits a concentrated, yellowish-white color, indicating a potentially older stellar population. Extending outwards from this central region are fainter, bluish arms or extensions. These extensions appear less structured and more diffuse than a tightly wound spiral galaxy. The bluer color suggests the presence of younger, hotter stars and ongoing star formation, especially at the tips of the extensions. There is a hint of asymmetry in the overall structure, potentially indicating past or ongoing minor gravitational interactions. No strong dust lanes or clearly defined spiral arms are visible. The galaxy appears relatively smooth with some disturbances in the disk, likely on-going star formation.
