The galaxy presents as a spiral type, exhibiting a well-defined disk structure. Two prominent spiral arms emanate from a central bulge region. The arms appear somewhat flocculent and display varying degrees of openness, with regions of both tightly wound and more loosely wound morphology. The bulge appears moderately sized, with a yellowish hue. Traces of active star formation are indicated by the bluish color interspersed along the spiral arms. Some asymmetry is detected, suggestive of minor gravitational interactions or internal disturbances. There is a possibility of a weak bar structure across the central region.
