The galaxy presents as a spiral morphology, with a visible disk structure. The disk exhibits a moderately inclined orientation relative to the line of sight. The galaxy's overall color profile suggests active star formation, most notable in the central and arm regions. There is evidence of spiral arm structures, with a flocculent appearance; they appear somewhat diffuse and not sharply defined. The central bulge appears smooth, possibly indicating an older stellar population concentrated at the core. There is a slight asymmetry in the distribution of light in the disk. The diameter appears to be relatively compact. Overall, this galaxy demonstrates characteristics of a relatively massive spiral galaxy undergoing active, ongoing star formation.
