The galaxy presents as a disk galaxy with a bright, concentrated central bulge. The overall color is bluish, suggesting a population of younger, hotter stars. Evidence of a spiral structure appears to be faint, perhaps due to viewing angle or intrinsic properties of the galaxy. 

The disk appears slightly warped or irregular. There's a possibility of minor tidal disturbances based on the fuzzy edges of the arms or an asymmetric shape. 

The central bulge exhibits a notably high surface brightness, indicating a high density of stars, possibly an active galactic nucleus, but further spectroscopic data is needed to confirm this.
