This galaxy exhibits a somewhat smooth morphology with indications of possible disk-like features. The central region presents a bright, concentrated core. Extending outward from the core, there appears to be a flattened structure, potentially indicative of a disk, though the smoothness of the light distribution suggests it is not a well-defined spiral structure. Faint irregularities or disturbances are possibly present. There is a slight asymmetry. No clear signs of a major merger are evident, but subtle features hint at minor gravitational interactions, although this could be noise. The galaxy's color profile displays a noticeable gradient, transitioning from a brighter, bluer hue in the inner regions to a redder periphery.
