The galaxy exhibits a morphology indicative of a spiral type. Spiral arms are visible, displaying a tightly wound structure in the inner regions that becomes more open in the outer areas. The arms are not very well defined, but some regions appear to be more well defined than others. The number of arms are difficult to define due to the overall structure. The central bulge is not very prominent, it seems to be on the smaller side with only a small region of the galaxy dominated by it. A hint of a bar structure may exist. Signs of possible merging activity are present, possibly with some minor disturbances. The disk is not edge-on. The color suggests a mix of stellar populations, with bluer regions possibly indicating ongoing star formation in the spiral arms, and yellower hues towards the central bulge implying an older stellar population. Overall, this is an interesting galaxy with a somewhat messy structure.