The galaxy presents as a spiral type, exhibiting distinct spiral arm structures. These arms are observed to be somewhat flocculent. There is no apparent central bar feature. The galaxy appears to have a prominent bulge with a moderately bright core. The overall color suggests an intermediate population of stars, with some regions of bluer colors indicating on-going star formation. No signs of major mergers or disturbances are readily apparent. There are no indications of an edge-on orientation.
