The galaxy presents as a flattened, disk-like structure, viewed at a significant inclination. A bright, concentrated central bulge is observed, transitioning outwards into a fainter, extended disk. The bulge exhibits a yellowish-white hue, potentially indicating an older stellar population. The disk appears bluish, possibly due to ongoing star formation or a younger stellar population. The morphology indicates an absence of spiral arm structures, though subtle irregularities and faint extensions are observed in the outer disk region. There are some small, compact sources that appear to be interacting. The overall light distribution suggests a relatively smooth profile, though the blue color is a little clumpy. Dust lanes cannot be clearly identified from the image.
