This galaxy appears to be a relatively small, faint object. Morphologically, the galaxy exhibits a somewhat disturbed structure. While a central bulge or core region is not immediately discernible, there does appear to be a relatively high degree of central concentration. Faint, diffuse extensions are visible, suggesting tidal interactions or possible ongoing merger events. The overall shape lacks definitive spiral arms or a clear elliptical form, pointing towards a possible irregular or peculiar classification. There is a hint of asymmetry in the outer regions, potentially indicating recent interaction with a smaller companion. The light distribution shows a notable blue component, which indicates active star formation, contrasting with redder regions that could be older stellar populations. Overall, the galaxy's morphology suggests a dynamic system undergoing evolutionary processes.
