The galaxy appears to be a disk galaxy, viewed at a significant inclination. There's a bright, concentrated central bulge or core region. The disk itself exhibits a mottled texture, which could be indicative of spiral arm structure, but it is not clearly defined. One region of the galaxy has some significant disturbance from a suspected merging event. The overall color suggests a mix of stellar populations, with some bluer regions possibly indicating younger, hotter stars and some redder regions possibly indicating older, cooler stars or dust.
