The galaxy presents as a moderately inclined, elongated, disk-like structure. It appears relatively smooth, with a subtle central bulge. The overall color is bluish-white, suggesting a population of younger, hotter stars. There is a slight color gradient from the center outwards, potentially indicating ongoing star formation in the disk regions. The morphology suggests that the galaxy is likely not currently undergoing any major merger events or significant tidal disturbances, although minor disturbances cannot be ruled out at this resolution. The elongated shape suggests a classification towards an edge-on spiral or a lenticular galaxy.
