The galaxy presents as an elongated, disk-like structure viewed at a steep inclination. It is yellowish in the central region, which likely indicates an older stellar population. This area appears relatively smooth and concentrated. Progressing outward from the core towards the disk, the color shifts to a bluer hue, suggestive of more recent star formation. The galaxy's disk does not exhibit well-defined spiral arms. The isophotes are tightly wound, resulting in a slender shape. There are no prominent dust lanes visible.
