The galaxy presents as a somewhat diffuse and face-on spiral structure. The central bulge appears bright and relatively smooth, with a slight elongation. The spiral arms are not well-defined, showing a flocculent morphology with patchy, less distinct arm segments. There's evidence of some blue color concentrated within the central region and some regions within the arms, potentially indicating ongoing star formation. Faint tidal tails are not obviously present, but there may be slight disturbances in the overall shape of the galaxy. The galaxy exhibits a moderate luminosity and is roughly two kiloparsecs in diameter. It is currently experiencing a relatively low rate of star formation and has a relatively low stellar mass.
