The galaxy presents as an elongated, disk-shaped structure viewed at a significant oblique angle relative to our line of sight. A central bulge is readily apparent, exhibiting a yellowish-orange hue, suggestive of an older stellar population and reduced star formation within this region. Surrounding the bulge is a flatter disk, which displays a more bluish tint, possibly indicative of ongoing star formation activity and a younger, hotter stellar population. 

The disk appears somewhat asymmetrical and possibly disturbed, hinting at past interactions or internal dynamic processes. While there are no clearly defined spiral arms evident at this resolution, subtle variations in color and brightness across the disk imply the presence of underlying structure. The overall smoothness of the light distribution suggests that any ongoing merging activity is either in its early stages or involves a minor companion galaxy not immediately apparent in the image.
