The galaxy presents as an elliptical morphology, exhibiting a smooth and relatively featureless structure. The central bulge appears dominant, displaying a yellowish-white hue, suggestive of an older stellar population. Moving outward from the core, the galaxy gradually fades into a fainter, more diffuse halo. There is a hint of a flattened shape, but it is difficult to observe any clear spiral arm structures. The overall color profile indicates a lower rate of recent star formation activity across the galaxy, with potentially ongoing but limited activity concentrated near the center. No apparent signs of a major merger event are visible.
