The galaxy presents a generally smooth appearance, with no readily discernible spiral arms or bar structure. It exhibits a somewhat elliptical shape, appearing moderately round rather than highly elongated. There may be some subtle disturbances in its morphology, possibly indicative of minor gravitational interactions. There is no sign of a major ongoing merger. The galaxy's color suggests active star formation, with a relatively high specific star formation rate. Overall, the galaxy appears to be a disk or irregular-type galaxy, potentially experiencing a period of moderate star formation.
