The galaxy presents a smooth, centrally concentrated morphology. The core exhibits a yellowish hue, indicative of an older stellar population. There is a slight elongation to its form, deviating minimally from a perfectly circular shape. Faint blue tinges are present in the outer regions, suggesting the presence of some younger, star-forming regions, although they are not dominant. There is no obvious evidence of strong spiral arms or a well-defined disk structure. Subtle disturbances may be present, but the overall impression is one of a relatively undisturbed system.
