The galaxy presents as a spiral type, exhibiting a prominent disk structure. A relatively small bulge is discernible at the galactic center, which seems to emanate yellowish-white light, indicative of an older stellar population. Prominent spiral arms emanate from the central region and appear loosely wound, showing a bluish tinge, potentially signifying active star formation regions. There are hints of dust lanes along the spiral arms which contribute to the overall structure. There is no evidence of tidal tails or distortions suggesting a significant recent merger event. The galaxy exhibits a moderate inclination relative to our line of sight, allowing the spiral structure to be partially observed.
