This galaxy appears to be a spiral galaxy, potentially observed edge-on, displaying a prominent central bulge and a fainter, extended disk. There is evidence of significant disturbance in the galactic structure. The disk exhibits asymmetries and irregular features that could be indicative of an ongoing or recent merger event. A substantial portion of the light from the galaxy is concentrated in the bulge region, which is relatively smooth and featureless. The disk itself shows a clumpy morphology, likely composed of areas of active star formation. The color of the disk appears to be bluer than the bulge, which is consistent with a younger stellar population.
