The galaxy presents as a somewhat elliptical structure, demonstrating a dominant central bulge. This bulge exhibits a smooth, concentrated light profile, suggesting a high stellar density composed primarily of older stellar populations. The surrounding disk, though less pronounced, displays a slightly bluer hue than the bulge, which may indicate the presence of ongoing, though modest, star formation within the disk regions. There are some faint disturbances on the outskirts, potentially caused by minor interactions, but it is mostly undisturbed. The galaxy as a whole displays a consistent structure. Overall, this galaxy appears to be a mature system in a later stage of evolution.
