The galaxy appears to be a spiral type, exhibiting well-defined spiral arms that emanate from a central, moderately sized bulge. The arms are not tightly wound, presenting a more open morphology. Within the arms, there are hints of star-forming regions, indicated by a slightly bluer hue and some clumpy substructure. The bulge itself presents a smoother, yellower color profile, suggesting an older stellar population. Overall, the galaxy displays evidence of ongoing star formation activity, with the spiral arms as the primary sites of this activity. The structure is not perfectly symmetrical, exhibiting a slight asymmetry that may be due to tidal interactions or internal dynamical processes. There is no strong evidence of a prominent bar feature in this image, although a subtle elongation may be present.
