The galaxy presents as a luminous, relatively smooth and centrally concentrated object. The morphology appears to be primarily elliptical, with a subtle deviation towards a more rounded shape rather than a highly elongated form. The dominant color is indicative of an older stellar population, with a noticeable reddish-yellow hue. There is a suggestion of some minor disturbances in the galactic structure, possibly indicative of past or ongoing minor interactions or internal dynamical processes. These disturbances don't suggest any major merging events. Based on its apparent size and luminosity, this galaxy is likely a massive system. Star formation appears to be minimal, consistent with a galaxy dominated by an older stellar population.
