This galaxy presents a generally smooth appearance, exhibiting a morphology leaning towards elliptical. Its shape is moderately elongated. The central region appears to be substantially brighter and more concentrated than the outer regions, suggesting a prominent bulge. There are no obvious signs of ongoing major merging events, though subtle disturbances cannot be ruled out definitively at this resolution. Color gradients suggest a population of older stars dominating the light output, particularly within the central bulge, with slightly bluer, younger populations possibly present in the less dense outer regions. 
