The galaxy presents a diffuse and somewhat amorphous structure. It lacks a clearly defined nucleus or spiral arms, appearing as a relatively smooth distribution of light. Its color is predominantly a muted blue-green, suggesting a mix of stellar populations. The outer edges fade gradually into the background, with no sharp cutoff indicating its boundary. There may be faint irregularities in the light distribution within the main body of the galaxy, hinting at potential tidal interactions or internal disturbances. The galaxy presents a low surface brightness, suggesting it is faint in its magnitude. Possible ongoing or recent mergers seem likely, considering the irregular morphology.
