The galaxy presents as a system undergoing a significant merger event. The primary body appears relatively smooth, with a concentrated central bulge exhibiting a yellowish hue, suggestive of an older stellar population. A secondary, smaller component is visible to the left, displaying a bluer tint, potentially indicating ongoing star formation within that region. There is a notable disruption of the morphology of both bodies, with tidal features and distortions indicating gravitational interactions. The overall shape is irregular, far from a regular spiral or elliptical morphology, further supporting the classification as an actively merging system. A notable portion of the light emitted is in the green and red wavelengths.
