The galaxy presents as a spiral type, with a prominent, moderately sized bulge at its center. The central bulge exhibits a yellowish-white hue, suggestive of an older stellar population. Extending outward from the bulge are loosely wound spiral arms. The arms exhibit a bluish tinge, hinting at regions of ongoing star formation and a younger stellar population. Two well defined spiral arms dominate the structure. The overall disk orientation appears to be relatively face-on, providing a clear view of the spiral structure. There is some evidence of minor tidal disturbances or interaction, but is not a significant disruption of the galaxy's overall morphology.
