The galaxy presents as a disturbed system, possibly undergoing a merger event. There appears to be an elongated structure with a bright central condensation, indicative of a galactic nucleus. Emanating from the central region is a less defined, fainter tail-like feature. This component displays a bluer hue, suggestive of ongoing star formation. The overall morphology deviates significantly from a regular elliptical or spiral form, pointing towards gravitational interactions or recent accretion events. Further spectral analysis is required to ascertain the composition, age, and metallicity of stellar populations within each component to better understand the galaxy's evolutionary history.
