The galaxy presents a somewhat amorphous morphology, suggestive of an elliptical or lenticular type, though there may be the presence of a disk. Its central bulge appears prominent and relatively bright, exhibiting a yellowish hue, indicating a potentially older stellar population with fewer young, massive stars. Extending outward from the core, the luminosity fades, with subtle hints of a disk-like structure. The outer regions display a faint, slightly bluer tint. The overall appearance suggests a system that may be undergoing some interaction or disturbance.&#x20;
