The galaxy exhibits a morphology indicative of a spiral structure, viewed at an oblique angle. A pronounced central bulge is apparent, with a concentrated luminosity. Faint spiral arms extend from the central bulge, suggesting a well-defined disk component. The arms have a clumpy texture, potentially indicating ongoing star formation regions, and they show a fragmented structure indicating either disturbances due to a merger or tidal forces. The overall color distribution suggests a mix of stellar populations.
