The galaxy presents as a well-defined, elongated, and somewhat flattened structure. A central bulge, appearing yellowish-white, dominates the galaxy's core. This area likely represents a high concentration of older stars. Extending outwards from the bulge is a disk that appears relatively smooth. Faint hints of spiral structure may be present within the disk, though the image resolution limits a definitive assessment. The disk exhibits a blueish tinge. The galaxy's overall morphology is most likely that of a spiral galaxy, observed at an oblique angle. There are no obvious signs of on-going major mergers or strong tidal disturbances, suggesting it is relatively undisturbed.
