The observed galaxy presents a complex morphology, appearing as a system of interacting components. A primary, relatively smooth and rounded component dominates the structure, exhibiting a bright, diffuse glow. This central region displays a yellowish-white hue, suggestive of an older stellar population. Adjacent to this, a smaller, more concentrated reddish-orange region is visible, potentially indicating a region of active star formation or a heavily dust-enshrouded nucleus. A distinct blue component is present, located peripherally to the main body. The presence of this component suggests a region of younger, hotter stars. The overall disturbed appearance of the system and close proximity of the components suggest that this galaxy is likely undergoing a merger or tidal interaction with a companion, inducing morphological disturbances and triggering localized star formation.
