The galaxy presents as a spiral type. It has a prominent, moderately sized bulge with spiral arms emanating outwards. The arms appear flocculent and somewhat patchy in their structure. There are two spiral arms. Dust lanes are visible within the spiral arms. There is a suggestion of a bar structure. The colouration suggests active star formation regions within the arms, and an older stellar population in the bulge, with the spiral arms appearing bluer in colour than the central bulge. The galaxy appears to be relatively undisturbed with a high degree of rotational symmetry.
