The galaxy presents a smooth, elliptical morphology. It is relatively compact, with a concentrated central bulge that dominates the overall structure. The light distribution appears uniform and lacks distinct spiral arm features or prominent dust lanes. A very faint hint of a disk-like structure may be present. The galaxy exhibits a yellow-red color gradient towards the center, indicating an older stellar population in the galactic core. There are no obvious signs of active galactic nuclei activity or strong ongoing star formation. Minor disturbances or tidal features are not readily apparent, suggesting that the galaxy is relatively isolated and undisturbed by major merger events. The roundness of the galaxy is somewhere between round and in between as it does not have an extreme cigar shape. 
