The galaxy exhibits a complex morphology, suggestive of an ongoing or recent merger event. The core presents a bright, somewhat amorphous structure, centrally concentrated. Faint tidal tails are not apparent, though the overall shape deviates significantly from a relaxed elliptical form. Several distinct luminous clumps are observed in the vicinity of the central region, some connected by tenuous bridges of light. There is evidence of asymmetric light distribution within the system. The color indices suggest a mix of stellar populations, with bluer components apparent and redder hues dominating the central regions. The galaxy displays a disturbed morphology, and the merging process might be responsible for its current irregular structure and intense central luminosity.
