The galaxy presents as an elliptical morphology, displaying a smooth, concentrated light profile. The central region exhibits a yellowish-orange hue, suggestive of an older stellar population. Moving outwards from the core, the color shifts to a more bluish-white, hinting at the presence of some younger, hotter stars, although these do not appear to dominate. There is no obvious spiral arm structure or prominent dust lanes visible in this image. The galaxy appears relatively undisturbed, lacking any significant signs of recent major mergers or tidal interactions, although there may be some minor disturbances in the outskirts.
