The galaxy presents as a somewhat diffuse object with a relatively smooth morphology. It does not show a prominent disk structure or spiral arms. There are some indications of subtle disturbances or features suggesting potential interactions or internal processes. The overall color of the galaxy leans towards the bluer end of the spectrum, which may indicate ongoing star formation. The object exhibits moderate roundness in shape, not appearing significantly elongated. There is no clear evidence of a major ongoing merger, however minor disturbances can be seen.