The observed galaxy presents as a disk galaxy viewed nearly edge-on. The central bulge appears prominent and luminous, exhibiting a yellowish-orange hue, suggestive of an older stellar population. The disk is visible as a thin, elongated structure extending from the bulge, with some evidence of slight warping or disturbance. The outer regions of the disk are considerably fainter, exhibiting a bluer color, which may indicate younger stars. There is no apparent presence of strong spiral arms within the disk.
