The galaxy presents as a face-on spiral system. The spiral arms are tightly wound, exhibiting a somewhat flocculent structure with areas of blue-ish tinge and a subtle distribution of star forming regions. The central bulge appears relatively small and not particularly prominent compared to the overall disk size. A stellar bar is not obviously apparent. There is no readily observed presence of a major merger event, though subtle disturbances could indicate a minor interaction or past interaction event. The overall color profile suggests a mixture of stellar populations, with the central bulge displaying yellower hues indicating older stars.
