The galaxy presents a disturbed morphology, suggestive of an ongoing or recent interaction or merger event. The primary structure is a somewhat elliptical shape with a bright, concentrated central region exhibiting a yellowish-white hue. A secondary, smaller component appears separated from the main body. The two seem to be linked by a faint bridge of material.  There's a noticeable disruption to the overall symmetry, with irregular extensions. Color gradients are subtle but visible, with a redder tint in the core of the smaller object. The overall light profile indicates a substantial stellar population, potentially obscured by dust in localized regions. The galaxy's diffuse outer regions are ill-defined.
