The galaxy appears as a yellowish-orange, moderately bright object. It exhibits a generally smooth morphology, appearing somewhat elliptical in shape, though with some possible irregularities indicating ongoing gravitational interactions. The light distribution suggests a concentration of older stellar populations. The apparent interaction suggests ongoing star formation, although this galaxy presents as a more evolved system. The galaxy is moderately sized. There is no discernable spiral structure or prominent dust lanes. The object is not perfectly circular, suggesting some degree of rotational flattening or tidal distortion. There is a clear merger happening here.
