The galaxy presents as an elliptical morphology, with a smooth, diffuse light profile lacking distinct spiral arms or a prominent disk structure. The galaxy appears nearly round. The color gradient suggests a concentration of older stellar populations toward the galactic center, presenting a yellowish hue. A faint, bluer tinge along the outer edges may indicate a low level of ongoing star formation within the galaxy. There are no apparent signs of major mergers or tidal disturbances, suggesting a relatively isolated evolutionary path. The overall appearance aligns with that of a mature galaxy, possibly on the red sequence.
