The galaxy presents as a spiral type with a prominent central bulge. The bulge exhibits a yellowish hue, suggesting an older stellar population. Spiral arms are clearly visible, extending from the central bulge. These arms are loosely wound, with a patchy appearance, indicating ongoing star formation regions mixed with older stellar populations. Two main arms are discernible, along with some fragmented and less defined spiral structures. There is a visible disturbance in the galaxy's structure that may be due to a gravitational interaction with another galaxy, suggesting that the galaxy may be undergoing a merging event. Dust lanes are observable along the inner edges of the spiral arms, attenuating the light from the stars behind them. The overall color profile of the disk suggests a diverse range of stellar ages, with bluer regions indicative of younger stars and redder regions associated with older populations. There is some evidence of a weak bar structure across the galaxy's center. The disk itself does not appear to be edge-on.
