The galaxy presents as a moderately bright, spatially extended object. It exhibits a relatively smooth, concentrated morphology, with a prominent central bulge. There is a distinct color gradient, transitioning from a bluer hue in the central region to redder tones at the periphery, which may be due to different stellar populations. A slight extension or plume of light is visible, potentially indicating a minor tidal disturbance or interaction with a smaller companion galaxy. The galaxy does not show strong evidence of spiral arm structures. Its intermediate roundness suggests it is likely an elliptical or lenticular galaxy, viewed at a small angle relative to its plane.
