The galaxy presents a structure indicative of an elliptical or lenticular morphology. It appears elongated, displaying a smooth light distribution, and little indication of spiral arms or significant dust lanes. There is a primary central bulge, which is slightly brighter than the surrounding disc, and appears to be a spheroid. The observed colour suggests a relatively older stellar population and low star formation activity within the galaxy. There is a possibility of a minor interaction with another small galaxy nearby, but is more likely an artifact of the survey.
