The galaxy presents as a spiral type, with a noticeable disk structure. Two prominent spiral arms are clearly visible, exhibiting a medium winding pattern. The central bulge appears relatively moderate in size. A bar structure is present, potentially classified as weak or no bar. Star formation is evident, as indicated by the bluer regions interspersed within the spiral arms. The overall morphology suggests a galaxy undergoing active star formation within its spiral arms and disk. There is no strong evidence of a recent or ongoing major merger event, although some minor disturbance may be present.
