The galaxy appears as a small, somewhat diffuse object. There is a slight elongation observed, suggesting a possible disk-like structure, but it is not well defined. The color appears to be primarily greenish-blue, possibly indicating recent star formation activity or a population of hot, young stars. There is no clear spiral arm structure or distinct central bulge visible. The overall morphology suggests a potentially disturbed or irregular galaxy, but the image resolution makes it difficult to discern finer details regarding tidal features or mergers. The galaxy's faintness suggests that it is either distant or intrinsically low in luminosity. Further spectroscopic analysis would be needed to determine its redshift and confirm star formation rates.
