The galaxy presents as a spiral type, observed at a slight angle from face-on. Distinct spiral arm structures are visible, tightly wound around the central bulge. The arms exhibit a mottled texture suggesting active star formation regions, which appear as slightly bluer knots within the arms. The central bulge is prominent, appears yellowish in color, indicating an older stellar population. The spiral arms appear somewhat indistinct and fuzzy, implying high redshift, or large distance. There appears to be no sign of merger activity or major disturbances in the galactic structure, the appearance is that of an unperturbed system. The dust lanes are not clearly visible in the image. The bulge dominates somewhat, though a substantial disc is evident. There may be a weak bar feature present within the central bulge, but is difficult to resolve. Overall, the galaxy exhibits the general characteristics of a classic spiral galaxy.
