The galaxy presents as a system with multiple interacting components. A dominant, relatively smooth, centrally concentrated component exhibits a primarily yellow-red hue, suggesting an older stellar population with reduced ongoing star formation. Positioned close to it, but clearly separate, is a region of bluer light, indicative of more recent and ongoing star formation. The overall morphology appears somewhat disturbed, potentially suggesting an interaction or merger event is in progress or has recently occurred. There is an indication that there are tidal features or dust lanes present. The structure is somewhat elongated, although it presents itself as being fairly round.
