The galaxy presents a complex morphology, suggesting a possible interaction or recent merger event. It exhibits a somewhat elongated structure, with a brighter, more concentrated central region and a fainter, extended component. A significant asymmetry is visible, with one side appearing more extended and diffuse than the other. This asymmetry may indicate tidal features resulting from gravitational interactions. The color distribution suggests a mix of stellar populations. The central region has a yellowish hue, potentially indicating the presence of older stars, while the outer regions appear somewhat bluer, which could indicate the existence of younger stellar populations. The overall form of the galaxy is significantly elongated, with a relatively high degree of flattening.
