The galaxy presents as a spiral type, viewed at an oblique angle. A prominent central bulge is observed with a yellowish hue, indicative of an older stellar population. Fainter spiral arms extend outwards from the bulge. They appear tightly wound. The blue color suggests areas of active star formation. The arms exhibit a slightly patchy structure. The overall morphology suggests a well-formed disk galaxy with ongoing star formation. The galaxy does not appear to be undergoing any major merging events or strong tidal disturbances. A bar might be present, however the resolution is not sufficient to determine whether it is strong, weak or absent.
