The galaxy presents a distinctly disk-like morphology, viewed at a significant inclination, appearing nearly edge-on. A central bulge is apparent, exhibiting a concentrated, yellowish-white luminosity, suggesting an older stellar population. Extending from the bulge are faint, bluish arms, more prominent on one side, indicative of ongoing star formation. Dust lanes may be present, though obscured by the inclination and image resolution. Overall the galaxy appears to be undergoing some sort of disturbance, visible through faint merging patterns.
