The galaxy exhibits a complex morphology characterized by a dominant, smooth, centrally concentrated component and a distinct, bluer, arc-like structure. The primary component appears relatively featureless, showing a gradual decline in luminosity from its core. The arc-like structure is significantly bluer in color than the central region, suggesting a population of younger, hotter stars or ongoing star formation. The overall shape is neither perfectly elliptical nor strongly disk-like. There may be some level of gravitational interaction or disturbance present, but is unlikely to be a major merger.
