The galaxy presents a centrally concentrated morphology, appearing largely smooth in structure with minimal discernible features. Its overall shape is somewhat elliptical but leans towards a more circular, less elongated form. There is a slight suggestion of a faint disk-like structure. The galaxy exhibits a pronounced central bulge that appears quite luminous, with a sharp falloff in light intensity toward the outer regions. The core region exhibits a high degree of blue light, indicative of recent star formation, that quickly falls off with distance from the galactic center. Although there are not enough features to observe the presence of spiral arms, the low estimated star formation rate and the smooth structure of the galaxy suggest it is likely an early-type galaxy, potentially an elliptical galaxy. The galaxy does not appear to be undergoing any major merging events or significant disturbances.
