The galaxy presents as a somewhat elliptical structure with a notable central bulge. The light distribution appears relatively smooth with an observed flattening. There is a subtle gradient in color, with the central region exhibiting a slightly yellower hue, potentially indicating an older stellar population. The outer regions appear bluer, which might indicate the presence of younger stars. There is faint evidence of a disk-like component, though its structure is not well-defined. No distinct spiral arms or bars are visible. Based on the light profile, it is likely an intermediate-mass galaxy. There seems to be little to no ongoing major mergers or disturbances evident in its morphology.
