The galaxy presents a complex morphology. It appears to be an interacting system, possibly in the early stages of a merger. One component is a relatively smooth, elliptical-like structure with a concentrated core, exhibiting a yellowish hue indicative of an older stellar population. The second component displays a more irregular and clumpy structure with bluish tinges, suggestive of ongoing or recent star formation. There's evidence of tidal features, possibly faint streams or bridges of material, connecting the components. The overall appearance suggests gravitational disturbance and disruption of the galactic structures.
