The galaxy presents as a spiral type, observed at a near face-on orientation. Prominent spiral arms are readily visible, exhibiting a multi-arm structure. These arms display a moderate winding, neither tightly wound nor overly loose. Star formation appears active within the arms, indicated by the presence of brighter, bluer regions suggestive of younger stellar populations. The central bulge appears relatively small compared to the overall disk size. No strong bar structure is immediately apparent. There is some evidence of asymmetry or minor disturbances within the galaxy's structure, although no major merger or interaction is evident. The galaxy exhibits a somewhat flocculent structure, with less sharply defined spiral arms. The overall color profile suggests a mix of stellar populations, with a slightly bluer hue in the disk compared to the redder bulge, consistent with ongoing star formation.
