The galaxy presents as a spiral galaxy, observed at a slight incline to our line of sight. The central bulge appears prominent and relatively bright, suggesting a significant population of older stars. The disk of the galaxy exhibits well-defined, tightly wound spiral arms. These arms display a bluish tint, indicative of ongoing star formation and the presence of younger, hotter stars. There appears to be some dust present within the disk, contributing to the patchy appearance of the spiral arms. The overall structure suggests no signs of major disturbance, merger, or tidal interaction, indicating a relatively isolated evolution.
