The galaxy presents as a spiral, potentially barred, exhibiting moderately defined spiral arms. A prominent bulge occupies the central region, contributing significantly to the overall luminosity. The disk appears inclined relative to our line of sight, with evidence of dust lanes along the spiral arms. A distinct color gradient is noticeable, transitioning from bluer regions within the spiral arms, suggestive of ongoing star formation, to a redder hue within the bulge, indicating an older stellar population. There appear to be disturbances or irregularities in the morphology of the arms, suggesting possible past merger events. The galaxy does not appear to be perfectly symmetrical.
