The galaxy presents as a largely smooth elliptical structure with a central bulge that appears slightly elongated along its major axis. The light distribution suggests a high degree of central concentration, transitioning smoothly outward. The overall color profile implies an older stellar population, characterized by a yellowish to reddish hue in the core, with bluer tones slightly visible in the outer regions. This suggests ongoing, but limited, star formation activity within the galaxy. There is a slight asymmetry to the light distribution in the outer regions, which could possibly indicate past interactions or minor disturbances. No strong spiral arm structure or prominent dust lanes are visible. Overall the galaxy appears to be in an isolated field and shows no definitive signs of recent, ongoing, or major merger activity.
