The galaxy presents a morphology indicative of an ongoing or recent merger. The central region exhibits a concentrated, yellow-white core indicative of an older stellar population. Several distinct components are visible, suggesting multiple interacting galaxies. The redder regions likely denote areas of enhanced dust obscuration or regions of recent star formation. Faint tidal features or extended diffuse light is not obviously detectable. The overall structure displays a disturbed morphology, deviating significantly from a simple elliptical or spiral form.
