This galaxy presents a distinct spiral morphology, characterized by a prominent disk. The disk appears not to be edge-on. Two spiral arms emanate from the central region, demonstrating a relatively well-defined, symmetric structure. The arms exhibit a moderate winding tightness. A subtle central bulge is visible, but not a dominant feature. There is some evidence of a weak bar structure. No significant interactions or mergers are readily apparent, although the appearance hints at minor disturbances. Star formation is likely occurring within the spiral arms, inferred from the coloration, though there does not seem to be strong evidence of high star formation. The galaxy appears to be of medium size and mass.