The galaxy presents as a somewhat diffuse, centrally concentrated object. It appears to be undergoing a merger or a significant gravitational interaction, displaying a distorted morphology with what seems to be tidal features extending from the central body. There is evidence of active star formation within these extended features, indicated by the bluish tints present. The central region exhibits a yellowish hue, potentially indicative of an older stellar population or significant dust obscuration. While not a clear spiral, the color variations and irregular features suggest some underlying disk-like structure that is being disrupted. The galaxy doesn't appear perfectly circular; it seems elongated with some degree of asymmetry.
