The galaxy presents as a spiral type, although the arms are tightly wound and somewhat difficult to discern clearly. There is a central bulge, with a moderate amount of its overall light concentrated there. Hints of spiral structure extend outward from the bulge, showing a subtle bluish tint, potentially indicative of ongoing star formation within the arms. The color suggests a mix of stellar populations, including younger, hotter stars contributing to the blue component. The disk itself appears relatively undisturbed, showing no signs of major mergers or significant tidal disruptions. The galaxy's overall morphology suggests a well-defined spiral structure in a relatively isolated state.
