The galaxy presents a largely smooth morphology. The central region is quite bright and appears relatively round. There is a slight elongation or flattening, but the overall shape is generally circular. No distinct spiral arms or bar structures are readily apparent. The color profile suggests a population of older stars, with a yellowish-white hue dominating the central bulge. There's a hint of bluer tones extending towards the outer edges, potentially indicating regions of more recent, albeit low-level, star formation. There are no obvious signs of significant tidal disturbances or ongoing major mergers.
