The galaxy presents as a single, relatively bright, central region. The morphology appears largely smooth with a hint of features. The galaxy exhibits a slightly elliptical shape. There appears to be two bright regions offset from the central point. The light from this galaxy ranges across the g, r, and z bands, suggesting the presence of a moderate amount of older stellar populations. It is estimated to be a high mass galaxy, with moderate star formation activity. The estimated size of the galaxy is roughly 7.7 kpc across. Based on visual inspection, it is possible that the galaxy may be in a merger phase or experiencing minor gravitational disturbances.
