The galaxy presents as an elliptical system, exhibiting a smooth and centrally concentrated light profile. It displays a generally round morphology, showing only slight elongation. The core region is characterized by a bright, yellowish-white hue, indicative of an older stellar population. Moving outward from the center, the color gradually shifts to a more subdued, blue-tinged halo, hinting at some ongoing, albeit low, levels of star formation activity at its outer edges. There is no apparent evidence of any major disturbances or merging events in its recent history, although there are some very subtle disturbances around the center.
