The galaxy exhibits a moderately elongated shape, appearing cigar-shaped. It appears to be a relatively massive galaxy, as inferred by its luminosity. It is primarily smooth in appearance with minimal disk-like features. It appears to be a galaxy without major disturbances or ongoing merger activity. The color suggests that the galaxy is composed of an older stellar population with a lower rate of on-going star formation. The overall structure indicates a galaxy nearing the end of its star forming period.