The galaxy presents as an elliptical-like morphology, exhibiting a smooth, centrally concentrated light distribution. There is some indication of a more compact nucleus within the broader galactic structure. The galaxy is observed to have a moderate angular size. Its light profile appears relatively featureless, lacking prominent spiral arms or other distinct substructures, although there is some possible minor disturbance in the overall form. Color indices indicate a redder overall color, possibly signifying an older stellar population, but there are tinges of blue, suggesting some recent star formation. The object appears somewhat rounded, with an axis ratio near unity, but possibly verging toward an 'in between' spheroidal and elliptical shape. There is a chance the object is involved in a merger with another object, or some minor gravitational interaction. 
