The galaxy presents as a relatively small and faint object. Overall, the galaxy's light profile appears smooth and diffuse, with a slight elongation. There is a hint of a possible disk structure, though the smoothness of the overall light distribution suggests a dominant spheroidal component. No strong spiral arm features or distinct star-forming regions are discernible. There may be some minor disturbances in the morphology, possibly indicating past or ongoing interactions with another galaxy or object, though a possible merger cannot be ruled out.
