The galaxy presents as a centrally concentrated object with an overall elliptical morphology, displaying a largely smooth structure. The central region exhibits a significantly higher luminosity, with a yellowish hue. A subtle gradient extends outward from the core, gradually decreasing in brightness. The outer regions appear less defined, displaying a slightly irregular shape with hints of faint, diffuse structures. There is no indication of prominent spiral arms or a distinct disk component. The galaxy appears relatively isolated, with no obvious signs of a major ongoing merger or tidal disruption.
