The galaxy presents as a faint, slightly elongated disk with a smooth light distribution. Its apparent shape is somewhere between round and cigar-shaped. A subtle suggestion of spiral arm structure may be present, however, the overall morphology appears relatively undisturbed. The galaxy exhibits a yellowish-white hue, suggestive of an older stellar population, but also contains traces of blue that could indicate younger stars. The galaxy appears isolated, with no obvious signs of interaction or merger activity. The estimated size suggests a galaxy of intermediate size.
