The galaxy presents as a diffuse object with a visually estimated effective radius of approximately 7 arcseconds. The overall morphology appears disturbed. The color distribution is uneven, with a prominent bright, greenish arc-like feature dominating the upper portion. This arc could indicate enhanced star formation or tidal interaction. A darker, reddish mottled region is observed throughout the body of the galaxy, possibly representing dust lanes or areas of older stellar populations. The galaxy does not exhibit a clear, defined nucleus or spiral arm structure. There are indications of potential tidal features or minor disturbances within the galactic structure that could point to interactions or merging events.
