The galaxy presents a spiral morphology. Two prominent spiral arms emanate from a central bulge. The arms exhibit a flocculent structure, appearing somewhat patchy and ill-defined. The winding of the spiral arms appears moderate, neither tightly wound nor exceptionally open.

The central bulge appears substantial, contributing significantly to the overall luminosity of the galaxy. There is evidence of a bar-like structure spanning a considerable portion of the bulge, which could be strong. The galaxy color appears to be a combination of blue in the spiral arms, which are bluer and areas of redder emission in the central regions. The blue color is suggestive of ongoing star formation within the spiral arms, while the redder color of the central region potentially indicates an older stellar population.

There is no evidence of significant tidal distortions or ongoing major merger events, but a minor disturbance could exist in the galaxy morphology. The galaxy appears largely undisturbed in its immediate environment.
