The galaxy appears as a well-defined elliptical structure. The central bulge is bright and concentrated, exhibiting a smooth, symmetrical profile. The outer regions show a gradual decrease in surface brightness, with a diffuse halo extending beyond the core. The galaxy is not perfectly spherical, showing a slight deviation towards a more elliptical shape, but still looks relatively rounded. There are no prominent dust lanes or spiral arm features visible. No obvious signs of a recent major merger event are detectable. Possible minor asymmetry or disturbances are not significant enough to indicate ongoing tidal interactions. Overall, it seems like a relatively undisturbed, evolved system. The color profile appears generally uniform, with a tendency towards redder hues, suggesting an older stellar population.
