The galaxy appears to be a spiral type, presenting a generally face-on orientation. It exhibits a distinct disk structure, with a central bulge that appears relatively small in comparison to the overall disk size. Two well-defined spiral arms emanate from the central region, winding moderately outwards. The arms are populated with regions of apparent star formation, indicated by the clumpy textures and slightly brighter areas within the spiral arms. There is a suggestion of a bar-like structure, with a faint elongation observed across the central bulge. There may be a slight tidal disturbance, but nothing particularly significant. The galaxy displays a blueish hue, suggesting the presence of a relatively young stellar population.
