The galaxy exhibits a disturbed morphology, suggestive of an ongoing or recent interaction. It appears to consist of two distinct, bright components in close proximity. The larger, primary component exhibits a yellowish hue, indicative of an older stellar population and reduced star formation activity. The secondary component, located just below it, is slightly fainter and more compact, and a similar color. A faint bridge of material, with slightly more blue tint, seems to connect the two components, hinting at tidal forces at play. There is no strong evidence of spiral arm structure or a well-defined disk, suggesting a transition towards a more spheroidal or irregular shape as a result of the interaction. The overall color profile and smoothness suggest this is a relatively massive system. The low star formation rate suggests an evolved system, potentially with ongoing quenching mechanisms.
