The galaxy presents as two distinct components: a central, spheroidal bulge and a surrounding disk. The bulge appears largely smooth and featureless, exhibiting a concentrated light profile. The disk, in contrast, is observed edge-on, presenting a flattened structure. The disk's color is notably redder than the bulge, possibly indicative of an older stellar population or increased dust obscuration. Some minor disturbance within the disk is suggestive of potential interactions or internal processes affecting its morphology. The galaxy's overall structure suggests a possible intermediate stage in morphological classification, transitioning from a disk-dominated to a bulge-dominated system.
