This galaxy presents as a complex structure exhibiting characteristics of an ongoing or recent merger. There appears to be a larger central component, relatively smooth in appearance. To the south, there are at least two distinct, luminous knots. These knots display more irregular morphologies, potentially indicative of tidal features or merging dwarf galaxies. The central component is more elliptical while the components to the south are more disk-like. Overall, the galaxy does not have a clear spiral or elliptical shape, possibly due to the merger dynamics. The galaxy exhibits a color gradient with the central region appearing slightly bluer than the outer regions and the knots appearing more orange. This may suggest an ongoing or recent burst of star formation, more concentrated in the knots.
