The galaxy presents as a moderately bright object, with a somewhat diffuse, centrally concentrated morphology. A significant portion of its light appears to originate from the central region, suggesting the presence of a bulge or nuclear component. The galaxy exhibits a slight blue hue, which may indicate ongoing or recent star formation, particularly in the outer regions. There is some irregularity visible in the outskirts. The object appears slightly elongated. Given the fuzziness of its features, this is either a distant or disturbed galaxy.
