The galaxy presents as a spiral type, with a relatively bright and concentrated central bulge. Two distinct, well-defined spiral arms emanate from this central region. The arms appear grand design, extending outwards in a loosely wound fashion.

The color distribution indicates active star formation within the spiral arms, suggested by bluer tints in the outer regions of the disk. The central bulge exhibits a more yellow to reddish hue, potentially indicative of an older stellar population.

A subtle bar-like structure may be present across the galaxy's core. The galaxy appears relatively undisturbed, with no obvious signs of recent major mergers, though minor asymmetries in the arm structure may suggest some past gravitational interaction. The disk is oriented nearly face-on, allowing for a clear view of its spiral structure. Overall, the galaxy exhibits a classic spiral morphology with ongoing star formation.
