The galaxy presents as a spiral type, viewed at a significant angle to edge-on but not quite face-on. I observe a prominent central bulge, though it does not dominate the overall structure. The spiral arms are clearly visible, exhibiting a tightly wound morphology, with some arms appearing more defined than others. The presence of at least two spiral arms are readily apparent. There is suggestion of a bar structure crossing the central bulge. The disk appears smooth. No major signs of ongoing merger events, though there may be minor disturbances in the disk that warrant further investigation.
