The galaxy presents a distinct spiral morphology. A prominent central bulge, slightly elongated, displays a yellowish hue, suggestive of an older stellar population. Emanating from this central region are several spiral arms, exhibiting a tightly wound structure. The arms are characterized by a bluish tint, indicating the presence of younger, hotter stars and ongoing star formation. The resolution limits a precise count, but several arms are clearly discernible. There is no obvious distortion or tidal features to suggest a recent major merger, though some minor asymmetries in the arm structure could imply minor interactions or internal disturbances. The galaxy appears to be viewed at a near face-on orientation.
