This galaxy appears to be a relatively small, faint object. It exhibits a somewhat irregular morphology, possibly indicative of a disk-like structure. The galaxy displays a bluish hue, suggesting the presence of younger stars. The color also suggests ongoing star formation activity within the galaxy, although perhaps at a low rate. There are hints of some disrupted structure, indicating the possibility of past minor disturbances, though the overall appearance is not that of a major merger event. The galaxy's light profile seems moderately smooth.
