Observed object exhibits an elongated morphology, appearing as a relatively flat and extended structure. The visible light distribution suggests a potential disk-like galaxy viewed at a high inclination angle. There is evidence of asymmetry within the galaxy, potentially indicative of tidal interactions or recent merger activity. A distinct, yet faint, feature is present, possibly representing a disturbed arm or tidal tail. The primary body of the galaxy demonstrates a gradient in light intensity along its major axis. The distribution of light along the disk appears somewhat clumpy, rather than smooth. The overall color appears reddish, which would suggest it may be an older galaxy.
