The galaxy presents as a spiral type, viewed at an angle slightly inclined from edge-on. A central bulge is evident, appearing relatively small in proportion to the overall disk size. The spiral arms are well-defined, exhibiting a grand design with two dominant arms that are loosely wound. The disk shows some irregularities, potentially indicating minor gravitational disturbances or ongoing interactions. The overall color profile of the galaxy appears slightly redder and there does not seem to be a strong presence of bright star-forming regions within the arms. There is a faint bar-like structure that could be present within the galaxy. 
