The galaxy presents as a disk-shaped system, seen at a significant inclination. The central bulge appears prominent and elongated along the disk's major axis. The color gradient suggests a population of older stars concentrated in the bulge, exhibiting a reddish hue. There's evidence of ongoing star formation within the disk, particularly on the lower side of the image, indicated by the presence of bluer regions possibly tracing spiral arm segments. Overall, the morphology suggests a spiral galaxy with characteristics of both a smooth component in the bulge and more actively star-forming regions within its disk. There is no obvious evidence of recent merging activity or major disturbances to the structure of the galaxy, though subtle asymmetries can not be ruled out with this image.
