This galaxy presents as a singular, fairly symmetrical object. The morphology is predominantly smooth, with a relatively high degree of roundness. The galaxy appears to be undergoing a merger, or may be experiencing minor tidal disturbances to its form. There is likely to be a central bulge that is surrounded by a less dense distribution of stars, dust, and gas. The color profile appears to show a mix of older stellar populations at the center and perhaps more recent stellar formation occurring elsewhere within the system.