The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a generally round morphology, with minimal indication of significant ellipticity. The core of the galaxy displays a bright, concentrated luminosity, suggesting a substantial central mass concentration. Moving outward from the center, the light gradually diffuses. There is some subtle indication of possible minor disturbance in the outer regions, however this is not very significant. Overall, the galaxy gives the impression of being relatively undisturbed. The color profile appears to be relatively homogenous across the body of the galaxy.
