The galaxy presents as an edge-on spiral system with a prominent, bright central bulge. The bulge exhibits a yellowish hue, suggesting an older stellar population. A flattened disk extends outwards from the bulge. The disk appears relatively smooth, showing minimal discernible substructure like prominent spiral arms or distinct dust lanes. The overall color gradient transitions from yellowish in the central bulge to a slightly bluer tone in the outer disk, possibly indicating ongoing star formation in those regions, although the activity appears subdued. The galaxy's light distribution suggests a significant fraction of its mass is concentrated in the central bulge. The galaxy doesn't exhibit any obvious signs of tidal distortions or interaction with other galaxies. Its structure appears generally undisturbed, suggesting relative isolation or stability.
