The galaxy presents a largely face-on orientation relative to our line of sight. Its structure suggests a spiral morphology, although the spiral arms are somewhat diffuse and not sharply defined. A central bulge is discernible, appearing moderately sized and exhibiting a smooth, concentrated luminosity. The overall color of the galaxy suggests ongoing star formation, with blue hues indicating the presence of young, hot stars. No strong bar structure is obviously visible. There is no evidence of a major merger. The overall visual impression is that of a galaxy with a mixed population of stars and an appreciable degree of ongoing star formation.
