The galaxy exhibits a prominent central bulge, appearing bright and somewhat spherical. The overall morphology suggests a spiral structure, although the arms themselves are not sharply defined. There is evidence of ongoing star formation activity, but it is not extensive. The disk appears relatively undisturbed with no signs of major mergers, but there are indications of some minor disturbances. A weak bar structure may be present within the central region. The overall appearance suggests a galaxy with a substantial stellar mass and moderate star formation rate.
