The galaxy presents as a relatively small, elongated system. Its color profile suggests a dominant older stellar population, with a discernible blue hue at its core. A disk is clearly visible, contributing to its lenticular shape. There is evidence of recent star formation, concentrated centrally within the galaxy. No significant tidal features or indications of major merger activity are readily apparent, though there may be some minor disturbances to the overall morphology. The primary axis of the galaxy is significantly longer than its minor axis. It is not especially round.
