The galaxy presents an overall elliptical morphology, with its major axis oriented horizontally in the image. The central region exhibits a bright, concentrated luminosity profile, likely indicative of a dense stellar population or active galactic nucleus. Proceeding outward, we observe a distinct color gradient, with the core showing a bluer hue that gradually shifts towards redder tones in the outer regions. This change suggests a potential age gradient in the stellar populations, with younger, hotter stars residing in the core and older, cooler stars dominating the periphery.

While the main body of the galaxy appears relatively smooth, there are suggestions of minor asymmetries or disturbances in the outer edges, possibly indicating past or ongoing gravitational interactions. A faint, extended halo surrounds the galaxy, blurring slightly into the background and further evidence of tidal stripping. Further examination is needed to determine whether these are genuine features or artifacts of the image processing. The galaxy is generally well-defined but shows some internal structure.
