The galaxy presents as a moderately bright object at a redshift of approximately 0.187. It appears relatively smooth in morphology, with a dominant spheroidal component. The overall shape is somewhere between round and cigar shaped. There may be a faint disk feature, although the spheroid appears to dominate the light profile. There is no readily apparent ongoing major merger activity, however, some minor disturbance can not be ruled out. Based on the color index, the galaxy appears to have a strong population of older stars as well as a modest amount of star formation.
