This galaxy exhibits a complex morphology, appearing as a system comprised of at least two distinct components. One component presents as a relatively smooth, centrally concentrated object with a yellowish-orange hue. There appears to be an area of decreased emission in the center. The other component, positioned nearby, shows a bluer color and less defined structure. This suggests the possibility of ongoing or recent interactions, perhaps a minor merger or tidal disturbance. The generally smooth appearance of the main body indicates it may be an elliptical galaxy, however the other component seems to indicate a disk like structure. There is evidence of moderate star formation activity.
