The galaxy presents as a moderately bright, elliptical-like structure. Its core is a concentrated region of high luminosity, appearing almost stellar in its central intensity. The overall color profile indicates a bias toward blue wavelengths, suggesting the presence of younger stellar populations. The galaxy's morphology is largely smooth, lacking prominent spiral arms or distinct features. The axial ratio suggests a flattened, but not highly elongated, shape. There is evidence of some minor disturbances, possibly indicative of past interactions or mergers. Some faint extensions are visible, implying tidal features or ongoing accretion processes. The light from this galaxy has been stretched by a noticeable amount as it journeyed towards us.
