The galaxy presents as a somewhat irregular, though overall smooth, structure. There is a noticeable degree of blending or possibly merging with one or more other galaxies, or perhaps a recent disturbance. The main body of the galaxy appears elongated, with an approximate size around 6 kpc. The shape falls somewhere between elliptical and disk-like, being relatively smooth in its light distribution but showing some faint features that hint at a disk. There are hints of differing stellar populations and some possible star formation ongoing in the galaxy. Overall, the galaxy appears to be in a state of transition or interaction, based on its morphology. The color indices imply that the galaxy hosts a mix of older and younger stars, and possibly ongoing star formation, although there is evidence the overall star formation is low. The galaxy is of moderate mass and luminosity.
