The galaxy presents an overall elliptical morphology with a smooth, concentrated light profile. The central region exhibits a bright, yellowish core indicative of an older stellar population. The outer regions of the galaxy appear more diffuse and exhibit a subtle disk-like structure. There's a slight color gradient from the center outwards, with the outer regions showing a bluer hue, potentially indicating some ongoing star formation, albeit at a low rate. No prominent spiral arms or major disturbances are visually apparent.
