The galaxy presents as a spiral type, exhibiting prominent, well-defined spiral arms. These arms are relatively tightly wound around a central bulge. The bulge appears moderate in size. Color variations are present, suggesting differences in stellar populations or dust content. The galaxy's morphology is dominated by the features of its spiral arms, indicating an active disk component. There is no apparent evidence of a major merger or significant tidal disruption. The galaxy's disk is oriented nearly face-on relative to the observer. A weak bar feature is suspected. Star formation is likely ongoing within the spiral arms.