The galaxy presents as a relatively smooth, centralized object. It exhibits a somewhat elliptical shape, leaning towards roundness. The light distribution appears concentrated towards the center, suggesting a prominent galactic bulge. There is a subtle color gradient, with a slightly bluer hue in the central region that fades to a redder color on the edges, which might point to older stellar populations in the outer regions of the galaxy. There's no obvious spiral structure or significant dust lanes visible in this image; the morphology suggests a galaxy without substantial current star formation. Indications of past or potential future merger events are negligible.
