The galaxy presents as a single, largely featureless entity with an elliptical morphology. The central region exhibits a concentrated luminosity, appearing brighter and displaying a warmer hue, possibly indicative of an older stellar population. Moving outward from the center, the light gradually diffuses into a halo. A faint blue tinge surrounds the halo which is suggestive of ongoing, albeit subdued, star formation in the outer regions. The galaxy appears generally undisturbed, lacking any strong signs of tidal interactions or major mergers. The shape is generally round, with only a slight elongation.
