The galaxy presents a generally smooth morphology. The central bulge appears largely spherical and dominates the galaxy's overall light output. There's a hint of a disk structure extending outwards, though it's not sharply defined. The galaxy exhibits a color gradient, appearing bluer in its outer regions and becoming redder toward its center. This color variation suggests a possible difference in stellar populations, with younger, hotter stars residing in the disk and older, cooler stars concentrated within the bulge. Some minor asymmetrical features are potentially present but may be due to noise. There are no visible signs of on-going major merger activity, though subtle disturbances might be indicative of past minor interactions.
