The galaxy presents as a relatively faint, diffuse object with a blue hue. It appears to have a somewhat irregular morphology, lacking a well-defined central bulge or distinct spiral arm structure. There's an overall patchy distribution of light within the galaxy's disk, indicative of possible ongoing star formation regions or dust obscuration. The galaxy doesn't show obvious signs of a strong bar, but some elongation along its major axis could suggest a weak bar or a more subtle, distorted structure. It also does not have a clear disk structure and might be an early-type or irregular dwarf galaxy. There may be minor disturbances or tidal features, indicating a possible past interaction or ongoing merger.
