The galaxy appears as a moderately bright, centrally concentrated object. It exhibits a roughly elliptical morphology with a smooth, diffuse profile and a slight elongation. The color distribution indicates a radial gradient, with a yellowish-white core transitioning to bluer outer regions. This might suggest a population of older stars in the center and younger stars toward the outskirts. While the overall appearance is relatively undisturbed, there is a hint of asymmetry in the outer regions, potentially indicating a past minor interaction or internal structure. Star formation appears to be occurring. There is no clear evidence of a strong, actively star-forming spiral structure or a major merger event.
