The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that appears yellowish-orange in color, suggesting an older stellar population. The surrounding halo is more diffuse and displays a subtle gradient in color, fading to a bluer hue towards the outer edges. This could indicate the presence of younger stars in the outer regions, possibly resulting from minor mergers or recent star formation. There seems to be a very slight distortion in the overall shape, hinting at a possible past gravitational interaction, although no prominent tidal features are visible. The overall color profile suggests a mix of stellar populations, with the core dominated by older stars and the outskirts exhibiting more recent star formation activity. The system does not appear to be undergoing a major merger or exhibiting strong signs of disturbance.
