The galaxy presents a flattened, disk-like morphology. A bright, concentrated central bulge dominates the structure, exhibiting a yellowish hue, suggesting an older stellar population. Surrounding this bulge is a fainter, extended disk. The disk appears relatively smooth and unstructured, showing only hints of spiral arm features or dust lanes. The color of the disk is somewhat bluer than the bulge, potentially indicating the presence of younger stars and ongoing star formation, even if at a low rate. The galaxy exhibits no obvious signs of a major merger, although the structure suggests the possibility of minor disturbances or past interactions. Overall, it appears as a relatively undisturbed disk galaxy with a prominent bulge, viewed at a moderate inclination.
