The galaxy appears to be a relatively smooth, elliptical type. It presents a concentrated central bulge, the light from this area is predominantly yellow, suggesting an older stellar population. There is a faint, diffuse halo surrounding the core, extending outwards. The halo region exhibits a gradual color gradient, transitioning from the yellower inner regions to slightly bluer tones in the outer parts. This may indicate ongoing star formation, or a younger stellar population, in these outer areas, albeit at a low rate. Overall, the galaxy seems well-defined, without any signs of significant tidal disturbances or major mergers. Its shape is fairly round, with only a slight deviation from perfect circularity. There are no prominent spiral arm structures or dust lanes visible.
