The galaxy presents a flattened, somewhat elongated profile, suggesting a disk-like structure viewed at a moderate inclination. The central region exhibits a bright, concentrated core, possibly indicating the presence of a galactic bulge or active galactic nucleus. Extending outwards from the core, a diffuse blue glow dominates the disk, indicative of ongoing star formation activity. The galaxy appears to be mostly uniform in color, however there is evidence of some patchy regions of redder hue near the disk of the galaxy, which may indicate regions of either dust obscuration, or older stellar populations. There is not clear evidence of spiral arms, nor signs of recent merging activity, however the edges of the galaxy are somewhat distorted and uneven, suggesting possible past gravitational interactions.
