The galaxy presents an overall flattened, elongated morphology, suggestive of a disk galaxy viewed at a high inclination angle, possibly edge-on. A prominent central bulge is visible, appearing yellowish in color, indicating a population of older stars. The disk component shows a bluer color gradient extending outward from the bulge, implying the presence of younger, hotter stars and ongoing star formation. One side of the galaxy has a faint, reddish region associated with it, possibly caused by dust obscuration or a region of ionized gas. There is some distortion present within the disk, particularly on the extreme edges of the galaxy, suggesting a potential past interaction or merger. There is a brighter area on the left edge of the disk of the galaxy. The structure does not appear to be perfectly smooth, with some irregularities in the distribution of light across the disk.
