The galaxy appears as a relatively smooth, elliptical-like object. It exhibits a concentrated central bulge with a gradual decrease in luminosity towards the outer regions. The galaxy appears a golden color, which may indicate the presence of an older stellar population. There is a faint hint of a disk structure embedded within the galaxy, but it is poorly defined. Overall, there are no clear signs of significant tidal disturbances or ongoing major merging activity. The smooth morphology suggests that it is likely a relatively undisturbed system with minimal star formation.
