The galaxy exhibits a primarily smooth morphology, with a noticeable lack of distinct spiral arms or a pronounced galactic disk. The light distribution appears centrally concentrated, suggesting a significant bulge component. The overall shape is roughly circular, deviating only slightly from a perfect ellipse. Faint, subtle features that may be indicative of minor disturbances can be tentatively identified. The color profile suggests a relatively evolved stellar population. There is a slight hint of asymmetrical light distribution in the lower portion of the galaxy.
