The galaxy presents as a spiral type, exhibiting a prominent central bulge. The bulge appears moderately bright and concentrated, with a yellowish hue. Two clearly defined spiral arms emanate from the central region, displaying a grand design morphology. These arms are relatively tightly wound and traceable for a significant portion of the galaxy's radius. Star formation is evident within the arms, indicated by bluer regions. A faint bar structure appears to be present traversing the bulge, which appears to be rather prominent. Overall, the galaxy appears to be relatively isolated, showing no major signs of interaction or ongoing merger activity, but there is a hint of minor distortion or tidal features possibly due to a minor interaction.
