The galaxy exhibits a compact morphology. It presents as a largely unresolved object, with no discernible spiral arms or bar structures evident within the available data. There are no indications of prominent dust lanes or regions of active star formation. The light distribution appears relatively smooth and centrally concentrated. There appears to be an adjacent object within the galaxy. There are some faint wispy features extending from the primary body, suggestive of tidal interactions or minor disturbances. Based on the observed features, the object could be potentially undergoing or have undergone a minor merging event with a less massive companion.
