The galaxy presents as a somewhat diffuse and centrally concentrated object. It exhibits a smooth overall structure with a hint of disk morphology, though not distinctly spiral. There is no evidence of a strong central bulge. The color profile suggests the presence of both older stellar populations and relatively recent star formation. The light is dominated by blue and green hues, indicating younger, hotter stars. There's a possible minor disturbance or slight asymmetry, but no major interactions or mergers are evident. The object has a relatively round appearance.
