The galaxy appears to be a disk galaxy, viewed nearly edge-on. A bright, concentrated central bulge dominates the core region, exhibiting a high degree of luminosity. The bulge fades into a surrounding disk component. Some distortion or tidal features may be present in the outer regions of the galaxy.

The central bulge is characterized by a predominantly smooth texture, indicating an older stellar population. The apparent color of the bulge is relatively uniform. 

The disk component appears relatively thin. There is some mottled texture with patches of color variation, which could indicate areas of active star formation.

Overall, this galaxy is intermediate in size. It appears to be relatively isolated, showing no prominent signs of a major ongoing merger.
