The galaxy presents as an elliptical morphology, exhibiting a smooth and somewhat elongated structure. The central region displays a concentrated luminosity, indicating a possible dense stellar population or active galactic nucleus. A gradual decrease in brightness is observed from the core outwards, suggesting a radially declining stellar density. The color profile appears relatively uniform with a slight yellow to orange hue throughout the galaxy, this suggests the presence of older stellar populations and minimal ongoing star formation. The overall appearance suggests a mature galaxy. There is no visual evidence of spiral arms, dust lanes, or significant irregularities in the galactic structure, further supporting its classification as an elliptical galaxy.
