The galaxy presents as a luminous, elliptical structure. Its core exhibits a high surface brightness, appearing predominantly yellow, suggestive of an older stellar population. The galaxy's morphology tends towards an intermediate elliptical shape rather than a perfectly circular one.

The outer regions display a more diffuse and subdued brightness, grading into a slightly bluer hue, implying the presence of at least some younger stars or perhaps some ongoing, albeit low-level, star formation within the galaxy's extended halo. No pronounced spiral arms or significant dust lanes are discernible. It appears to be fairly undisturbed, with no obvious signs of a recent major merger event. The overall structure suggests a system that is relatively relaxed and evolved.
