The galaxy presents a complex morphology, exhibiting features of both a smooth spheroid and a more irregular, possibly disk-like component. A bright, concentrated central region dominates, surrounded by a fainter, elongated structure. There appears to be evidence of some disturbance in the overall form, potentially indicating an interaction or recent merger event, marked by faint extensions or tidal features. The color distribution suggests variations in stellar populations and/or dust content within the galaxy. The core appears to be bluer and has a strong green tint.
