The galaxy presents as an irregular object with a disturbed morphology suggestive of an ongoing or recent merger event. A dominant, central component exhibits a diffuse, yellowish-white hue, possibly indicating a significant population of older stars. Distinct features include a second region of concentrated light located a short distance from the primary body. This secondary component appears less luminous and slightly redder. Tidal tails or extended arcs of stellar material are not clearly discernible. The overall shape deviates significantly from a typical spiral or elliptical structure, suggesting strong gravitational interactions have disrupted the original morphology. There appears to be a small, compact object located to the left.
