The observed galaxy presents as a flattened, disk-like structure seen nearly edge-on. A prominent central bulge dominates the galaxy's core, exhibiting a smooth and rounded morphology. The bulge appears to be primarily composed of older stellar populations, as indicated by its yellow-orange coloration. A faint disk extends outwards from the central bulge, with a significantly bluer hue, suggesting ongoing star formation within the disk. The galaxy exhibits a relatively smooth overall appearance, without any obvious signs of major mergers or strong tidal disturbances. Subtle irregularities in the disk's outer regions could indicate minor disturbances or interactions. The absence of bright, distinct spiral arms suggests a more flocculent or less well-defined spiral structure. The galaxy's elongated shape and relatively high disk-to-bulge ratio are consistent with a classification as a late-type spiral or lenticular galaxy.
