The galaxy presents as a spiral type. Its arms are tightly wound around a prominent, moderately sized bulge. A bar structure appears to run through the galaxy's center, influencing the spiral arm morphology. There is evidence of ongoing star formation, with regions of bluer light concentrated within the spiral arms. The galaxy does not show obvious signs of major mergers or significant tidal disturbances in its overall structure, although some minor disturbances are difficult to rule out at this resolution. The spiral arms are somewhat difficult to fully discern in terms of their precise number.
