The galaxy presents as a disk galaxy, observed nearly edge-on. Evidence of a bulge is not readily apparent. The disk exhibits a moderate degree of dust obscuration, though distinct dust lanes are not resolvable. Stellar populations within the disk show a range of ages, with some areas exhibiting bluer colors, indicative of ongoing star formation. The overall color profile suggests intermediate star formation rates. There is no strong visual evidence of a recent major merger, or a strong tidal disruption event. The galaxy is moderately luminous. The galaxy has an apparent size of approximately 10 kpc.
