This galaxy presents as a relatively small, elongated object. Its overall color appears bluish-white, suggestive of a stellar population with a significant proportion of young, hot stars. The galaxy's light distribution appears fairly uniform, with a subtle central condensation that may indicate a slight bulge. Faint and diffuse extensions can be seen, indicating that it may be a disk galaxy. No distinct spiral arm structures are apparent, but the disk appears to be slightly disturbed or irregular. This distortion suggests a recent interaction or merger. Overall, the galaxy is faint, indicating that it is far away, relatively small, or of low luminosity. The image suggests that this is a relatively faint and potentially disturbed galaxy, possibly a low-mass spiral or irregular galaxy undergoing interaction.
