The galaxy appears to be undergoing a significant merger event. The morphology exhibits a complex structure, with indications of tidal interactions and gravitational disturbances. A dominant, roughly spherical component is visible, exhibiting a reddish hue, suggestive of an older stellar population. Connected to this component is another distinct, less concentrated region with a slightly yellower color, possibly indicating a different stellar population or ongoing star formation. A third object, of a similar yellower color, appears slightly off center from the two primary components, which could be a dwarf galaxy or an independent bright region of star formation. Overall, the light is not evenly distributed, and this galaxy appears to be morphologically disrupted, with potential asymmetries. The relatively smooth appearance of its primary components suggests that it is an elliptical galaxy undergoing a merger.