The galaxy presents a generally smooth morphology, appearing as a single, concentrated object rather than showing distinct spiral arms or a well-defined disk structure. Its overall shape tends towards roundness, with a slight elongation potentially present. The galaxy exhibits a color gradient, transitioning from a yellower central region to a bluer outer halo. This color variation may indicate differing stellar populations or dust content across the galactic structure. There is no apparent major disturbance of the galaxy's structure and no evidence of an ongoing major merger event. A slight asymmetry in its light distribution suggests a possible minor interaction or disturbance.
