This galaxy exhibits a clear spiral structure, with prominent arms extending from a central bulge. These spiral arms appear somewhat patchy, suggesting ongoing star formation regions interspersed with older stellar populations. The bulge component appears moderately sized in comparison to the overall disk. There may be a weak bar feature present within the central region of the galaxy. The disk itself does not appear perfectly face-on, exhibiting a slight tilt that gives it an oval shape. The image hints at possible minor tidal disturbances or interactions, which could be influencing the star formation and morphological characteristics.
