The galaxy presents as a faint, elongated structure. Its core appears bright and somewhat yellow, suggesting an older stellar population dominating the central region. Fainter, bluer hues extend outwards from the core along the major axis, indicative of possible recent star formation activity in what appears to be a disk-like structure. The disk is not well-defined, appearing somewhat diffuse and patchy. The overall morphology is reminiscent of a spiral galaxy viewed at a high inclination or potentially an elliptical galaxy with a flattened shape. There are no obvious signs of strong tidal disturbances or mergers; however, a mild asymmetry is noted in the outer regions of the disk, hinting at a potential minor interaction. The galaxy's moderate redshift implies it is a distant object.
