The object in question appears to be a disk galaxy, observed at an oblique angle. There is a bright, concentrated central bulge, which is slightly elongated along the major axis of the galaxy. The disk component is visible and appears relatively smooth. 

Evidence suggests a possible interaction with another object. A slight asymmetry is observed within the main body of the galaxy, hinting at a potential minor disturbance.

The color profile indicates a higher concentration of bluer light in the central regions and along the edges of the disk, suggesting active star formation. The redder hues are primarily confined to the more central regions, perhaps indicating a population of older stars in the bulge. 
