The galaxy presents as a spiral type, with a relatively bright, concentrated central bulge. The disk is clearly visible, displaying prominent spiral arm structure. These arms are not tightly wound but rather appear more open and grand in design. There are signs of active star formation within these arms, noticeable as bluer regions dispersed throughout. Dust lanes appear to be interspersed within the arms, obscuring some of the light. There is a slight visual asymmetry to the spiral structure, potentially indicating past or ongoing interactions. The galaxy is observed nearly face-on. Overall, it presents as a reasonably massive galaxy with a moderate bulge and active star formation within its spiral arms.
