The observed galaxy presents a generally smooth morphology, with the majority of classifications indicating it as such. It appears nearly circular in shape, deviating slightly from perfect roundness. There is a suggestion of a slight perturbation in the overall structure; however, no major merger events or significant disturbances are readily apparent. The galaxy exhibits a subtle color gradient, with a central region appearing more yellow or gold, potentially indicative of an older stellar population concentrated in the core. The outer regions appear somewhat bluer, suggesting the presence of younger, hotter stars, although this feature is less pronounced. Overall the galaxy is relatively compact.
