The galaxy presents as a disk galaxy, viewed at a high inclination, appearing almost edge-on from our perspective. The disk exhibits a bright, concentrated central bulge, surrounded by a fainter, extended disk. Evident within the disk are structures that are consistent with spiral arm features, although the high inclination complicates their clear identification. These features appear somewhat disturbed. Star formation appears to be present in the spiral arms, indicated by a blueish hue. The galaxy has a moderately high estimated stellar mass. There is a noticeable degree of asymmetry or distortion in the overall structure, possibly indicating a past or ongoing interaction or merger event. There are regions of diffuse, fainter emission extending outward from the main disk, which may be tidal debris resulting from such an interaction. The data suggests this galaxy could be undergoing some merging event, though the magnitude is not clear, and star formation is likely occurring.
