The galaxy appears to be an elliptical galaxy with a generally smooth morphology and a high degree of central concentration. The core of the galaxy is noticeably brighter than the surrounding area, indicating a dense stellar population. The color profile suggests a relatively old stellar population, with a slight shift towards redder wavelengths in the central regions.  There is no obvious disk structure or spiral arms. The overall shape is generally round, showing minimal signs of tidal disturbances or recent major mergers. Faint, diffuse outskirts are visible, gradually fading into the background sky. These outskirts appear to be relatively smooth, consistent with the light distribution of an elliptical galaxy. Overall, the galaxy presents as a relatively undisturbed, evolved system.
