The galaxy presents an overall smooth morphology, indicative of a relatively evolved system. The light distribution suggests a centrally concentrated structure with a diffuse, extended halo. The central region is bright and appears yellowish-white, transitioning outwards to a fainter, bluish halo. There is very little resolved structure, such as distinct spiral arms or prominent dust lanes, suggesting a predominantly old stellar population. Faint disturbances are observed on the outskirts of the halo. Overall, the object is generally round in shape, with a slight elongation along one axis. There is very little ongoing star formation.
