The galaxy presents as a relatively smooth, elliptical-like structure with a bright, concentrated central bulge that appears slightly elongated. The color distribution suggests an older stellar population, with the bulge exhibiting a yellowish-white hue indicating evolved stars. The outer regions fade into a less defined halo, with subtle hints of reddish tones, possibly indicating regions of dust or older, redder stars. There is little evidence of spiral arms or active star formation regions. Overall, the galaxy appears well-defined and relatively undisturbed.
