The galaxy presents as a somewhat elliptical structure, exhibiting a noticeable bulge in its central region. The core appears luminous and concentrated, indicating a high stellar density. The color profile suggests a slightly redder hue in the core region, likely due to the presence of older stellar populations. Moving outwards from the core, the galaxy gradually fades, displaying a bluer color. The outer regions are less defined, hinting at a smoother distribution of stars and gas, with possibly a weak disk-like structure. There is a very slight visual disturbance within the galaxy, possibly indicating a minor interaction or internal activity, but otherwise the system looks relatively undisturbed. Overall, the galaxy appears to be relatively massive.
