The galaxy presents as a disk galaxy, viewed nearly edge-on. A prominent central bulge is observed, showing a concentrated, yellowish hue. This suggests an older stellar population dominating the core. The disk appears elongated and relatively thin, extending outward from the central bulge. The outer regions of the disk display a bluish tint, indicating the presence of younger, hotter stars and potentially ongoing star formation. Some degree of dust lane obscuration is suggested along the galactic plane, though it is not drastically pronounced. No major merger events are visually apparent, although subtle asymmetries might hint at minor gravitational disturbances. The bulge shape appears rounded rather than boxy. The galaxy appears to be relatively isolated, without any nearby companion galaxies visibly disrupting its structure.
