This galaxy exhibits a morphology consistent with a disk galaxy, presented nearly edge-on from our vantage point. The primary light concentration is centrally located within the disk, appearing somewhat diffuse and lacking sharp definition, which may indicate the presence of a bulge. The light distribution along the disk shows considerable asymmetry. One side displays a gradual fading, while the opposite side features a brighter, more abrupt truncation, possibly indicative of interactions with a companion galaxy or internal dust obscuration. There appears to be a secondary region of light concentration located along the disk, offset from the central bulge, which could be a result of asymmetrical star forming processes. The overall color profile suggests a moderate redshift, with redder tones dominant, indicating an older stellar population and potentially lower rates of ongoing star formation. Subtle irregularities are observed within the disk, which are consistent with minor gravitational disturbances or past merger events.
