This galaxy appears to be a relatively small, late-type system, likely a dwarf galaxy. The main body exhibits a somewhat diffuse and irregular morphology, with a noticeable blue hue, suggestive of ongoing or recent star formation. There are what appear to be multiple distinct, bright blue knots scattered within the galaxy, likely regions of intense star formation. Based on these properties, the galaxy is likely low mass, with a lower star formation rate overall. The presence of these distinct knots, as well as its asymmetrical shape, suggests possible interactions or disturbances in the system's recent past. There are no clearly defined spiral arms or central bulge present.
