This galaxy exhibits a prominent disk structure. Spiral arms are discernible, though they appear somewhat flocculent and not tightly wound. The arms display a mottled texture, suggestive of active star formation regions. The central bulge appears moderate in size and brightness, contributing a significant fraction of the galaxy's overall luminosity. There are visual features suggesting a possible minor interaction or tidal disturbance, though a clear merging event is not obvious. The galaxy shows characteristics indicating ongoing or recent star formation activity, potentially with a low rate of star formation. The galaxy's disk is not viewed edge-on; it is seen at an angle that allows the spiral structure to be distinguished. The color gradients across the galaxy suggest varying stellar populations, with bluer regions potentially indicating younger stars. The morphological features of the galaxy suggest it is an intermediate spiral type.
