The galaxy presents as a centrally concentrated, elliptical-like structure with a smooth, diffuse appearance. A distinct, reddish core is evident, suggesting a high density of older stellar populations or significant dust obscuration in the central region. The outer regions exhibit a bluer hue, possibly indicating the presence of younger stars or a lower dust content relative to the core. There is little to no evidence of spiral arms or other distinct morphological features; the overall shape is quite regular and undisturbed. Faint extended emission is barely perceptible surrounding the main body of the galaxy, making it unclear how far the object reaches into space. There is no clear indication of any ongoing major merger activity, though slight asymmetries or subtle tidal features cannot be ruled out. The light appears to be spread evenly with little in the way of knots of high stellar density. 
