The galaxy presents an elongated, cigar-shaped morphology. A central bulge region is evident, exhibiting a concentrated, yellowish-white hue, suggestive of an older stellar population. Extending outward from the bulge is a fainter, disk-like structure. The disk appears relatively smooth, with some subtle variations in color. The blueish tones in the disk, particularly at the outer edges, imply the presence of younger, hotter stars and ongoing star formation. No obvious spiral arm structures are apparent within the disk. There seems to be a slight warp or tilt relative to our line of sight. No major or disruptive merging events are visible in this image, suggesting that the galaxy is relatively undisturbed.
