The galaxy appears to be undergoing a merger or interaction with at least one other galactic object. The primary galaxy exhibits a generally smooth morphology, with a slightly elliptical shape, but with significant disturbance in its structure likely from ongoing tidal forces. A possible tidal bridge or arm of material extends toward the secondary object. The main galaxy displays a dominant central bulge with moderate color, hinting at a population of older stars. There may be some evidence of ongoing star formation in the disturbed region, indicated by the presence of some bluer colors.
