The galaxy presents as a relatively face-on spiral galaxy, exhibiting a well-defined disk structure. Two prominent spiral arms emanate from the central region, displaying a medium winding pattern, tightly wrapped around the central bulge. The arms appear asymmetric, with varying intensity along their length.

A distinct central bulge dominates the galaxy's core, suggesting a significant population of older stars concentrated in this region. A pronounced bar structure traverses the galaxy's center, influencing the spiral arm morphology. The disk shows clear signs of active star formation, seen through the enhanced blue emission and patchy regions along the arms. Overall the light emitted by the galaxy suggests it falls within an intermediate mass range, with ongoing star formation in its spiral arms. The galaxy appears to be relatively undisturbed, without significant signs of interaction or recent merger activity.
