The galaxy presents as a relatively compact object, exhibiting a generally smooth morphology. The core is bright and concentrated, suggesting a significant stellar density. A slight elongation is observed, deviating from a perfectly circular shape. There is evidence of a possible merger, with some irregularity or disturbance, as shown in the image. Color gradients are present, with a bluer hue in the inner regions transitioning to redder tones in the outer regions.
