The galaxy presents as a spiral galaxy with a moderate inclination relative to the observer's line of sight. The central bulge appears relatively prominent and exhibits a smooth, concentrated luminosity profile, indicating a likely population of older stars. Distinct spiral arms are visible, exhibiting a multi-armed structure. Star formation appears to be actively occurring within the spiral arms, indicated by the presence of blueish clusters. The arms are not uniform, showing areas of high star density. There's evidence of tidal disturbances or possible ongoing interactions, with visible asymmetrical distortions in the outer disk, but these could also be due to internal dynamics.
