The galaxy presents as a disk-shaped system, inclined at a moderate angle to our line of sight. A central bulge is apparent, exhibiting a yellowish hue suggestive of an older stellar population. Surrounding the bulge, a flattened disk structure is observed. The color of the disk transitions from yellow-green in regions close to the central bulge to a blueish tint at the outer edges, likely indicating the presence of younger, hotter stars and regions of active star formation further from the center. Some asymmetry is present in the outer disk, possibly indicating a gravitational interaction or recent merger event. Patches of redder hues are also present, indicating areas with dust. 
