The galaxy presents as a spiral with a relatively face-on orientation. The spiral arms are well-defined and extend outwards from a central bulge region. Blue color is apparent throughout the galaxy, including the arms, suggesting the presence of younger, hotter stars. The central bulge shows a slightly more yellow tint, indicating a population of older stars in this area. The arms show evidence of active star formation regions, marked by clumpy structures with higher concentrations of blue light. There is a hint of a bar structure present in the center of the galaxy, though it is not prominently defined. The galaxy shows some signs of possible interaction or disturbance. The spiral arms seem slightly distorted or uneven in their distribution.
