The galaxy presents as a single, centrally concentrated object with a generally smooth appearance. Its overall form is elliptical, appearing nearly round. There is a subtle color gradient, with a bluer hue concentrated towards the galaxy's core, suggesting the potential presence of younger, hotter stars in that region. The outer regions of the galaxy appear redder, indicative of an older stellar population. No prominent spiral arms, bars, or other distinct features are readily apparent in this image. The overall impression is that of a relatively undisturbed system, without signs of ongoing mergers or major tidal disturbances.
