The galaxy presents as a disk galaxy, viewed at an intermediate inclination. Its overall color appears bluish-white, indicative of a moderate population of younger, hotter stars. A notable feature is a ring-like structure exhibiting a strong green emission, possibly from ionized gas. A dust lane or some other form of obscuration is visible across the central region of the galaxy. The galaxy's morphology is somewhat disturbed, possibly indicating a previous or ongoing interaction with another galaxy. Overall the galaxy is an actively star forming system with signs of a recent merger. 
