The galaxy presents a disk-dominated morphology with a prominent spiral structure. The spiral arms are clearly visible, exhibiting a grand design with what appear to be several arm segments emerging from the central bulge region. These arms display varying degrees of pitch angle; some appear more tightly wound, while others are more open. Star formation activity is suggested by the clumpy nature of the spiral arms and bluer hues interspersed within the arms. The central bulge is noticeable but does not dominate the overall light profile of the galaxy, appearing relatively compact and yellowish in color. There appears to be a possible merger event or tidal interaction evident in the warped structure of at least one spiral arm. This distortion indicates ongoing gravitational disturbance.
