This galaxy presents a flattened, disk-like morphology, consistent with a spiral or lenticular galaxy. The central bulge appears moderately prominent and has a yellowish color, suggesting an older stellar population. Two distinct spiral arms appear to emanate from the central bulge, tracing a generally open winding pattern with a medium pitch angle. The arms exhibit some clumpy regions of bluer light, indicative of ongoing star formation within these areas. The overall disk structure reveals minimal signs of major tidal distortions or interactions, although there may be a hint of minor disturbance. A strong bar feature is present. The dust lanes are not clearly visible, suggesting a relatively face-on orientation and/or low dust content.
