The galaxy presents a generally smooth, elliptical morphology. The core exhibits a concentrated, bright luminosity, with a distinct reddish-orange hue indicative of an older stellar population. The surrounding halo gradually fades in intensity, showing a more yellowish color profile. There is little to no evidence of spiral arm structures or significant dust lanes. Overall, the galaxy appears to be a relatively undisturbed, mature system with minimal signs of recent or ongoing mergers or major disturbances. Its shape is closer to an ellipse, and the galaxy has the appearance of being quite massive. Given the light profile, star formation is likely very low in this galaxy.
