The galaxy presents as a faint, relatively small, disk-shaped structure with an intermediate inclination. It is slightly elongated along its major axis. The disk exhibits some features suggesting structure, although a smooth component is also apparent. A faint central bulge may be present, but it is not particularly prominent. There's a possibility that a minor disturbance is affecting the disk structure. The colour suggests that the galaxy has populations of both younger and older stars, with a low rate of star formation. No strong signs of merging activity or major disturbances are visible. The stellar mass of this galaxy is in the high range.
