The galaxy presents as a largely featureless, elliptical-like structure with a smooth light distribution. The core exhibits a concentrated, bright, yellowish-white hue, suggesting an older stellar population. The galaxy fades into a less luminous extended halo with a reddish tinge as it extends outward from the core. A slight asymmetry is present in the distribution of light within the halo, which indicates a possible ongoing interaction or disturbance. Based on the color profile and general morphology, this galaxy appears to be an evolved system with a moderate mass and a low rate of star formation. A disk may be present, though it is not easily discernible. There appears to be no major merging occurring.
