The galaxy presents a largely smooth morphology, appearing elliptical in shape. A concentration of light emanates from the central region, suggesting a prominent galactic nucleus. The color profile transitions from reddish in the core to a slightly greener hue in the outer regions, possibly indicating variations in stellar populations or dust content. The overall structure lacks any apparent spiral arms or significant disk features, further supporting its classification as an elliptical galaxy. There are no obvious signs of ongoing major mergers or tidal disturbances in the immediate vicinity, although some minor irregularities or faint extensions cannot be entirely ruled out due to the image resolution. The galaxy appears relatively isolated within its field.
