The galaxy presents as a spiral galaxy with a moderately sized bulge. Prominent spiral arms are clearly visible, tracing a grand design pattern with primarily two major arms. The spiral arms show a medium winding, neither tightly wrapped nor extremely loose. Within the spiral arms, one can observe a distribution of star forming regions or areas of heightened luminosity, suggesting active star formation. A bar structure seems to bisect the bulge, oriented lengthwise and extending into the disk. The colouration indicates a mix of stellar populations, with a generally older stellar population within the central bulge and disk, and hints of younger, bluer stars populating the spiral arms. There is no discernible sign of a major ongoing merger, although there might be some minor disturbances in the morphology of the outer disk. The galaxy is relatively well-defined, with a clear separation between the galactic structure and the background sky.
