This galaxy presents as a disk galaxy, viewed nearly edge-on. The overall morphology is suggestive of a significant disturbance, potentially a merger event. The central region appears brighter and more diffuse, possibly indicating a bulge, although this is obscured by the edge-on orientation. Extending outwards from the central region are fainter, elongated structures that may be tidal tails or distorted spiral arms. These structures appear asymmetric, supporting the possibility of past or ongoing gravitational interaction. Dust lanes appear likely, running lengthwise in the disk, although the low resolution makes their characterization difficult. There may be a companion galaxy involved in the interaction. The color profile seems consistent, with no drastic changes or evidence of substantial star formation outside the disk. The central region appears yellow.