The galaxy presents a largely smooth, elliptical morphology. Its central region exhibits a brighter, concentrated luminosity, which gradually diminishes towards the outer edges, with some hints of a slight disc structure. The color profile suggests a relatively older stellar population, with a yellowish hue dominating the core and a subtle shift towards redder tones in the periphery. There are minimal signs of active star formation apparent in the image. No significant dust lanes or spiral arm structures are discernible. There may be some minor disruption present as well.
