The galaxy exhibits a spiral morphology, characterized by relatively tightly wound arms emanating from a central bulge. The spiral arms display variations in luminosity, suggesting an ongoing star formation activity and differential distribution of interstellar dust. The central bulge appears moderately prominent, indicating a transitional stage between a disk-dominated and bulge-dominated system. The galaxy does not appear to be strongly barred. No major merger events are apparent, although the possibility of a minor interaction cannot be entirely excluded due to subtle disturbances in the outer regions of the disk. The orientation of the galaxy is somewhat inclined relative to our line of sight, providing a partially obscured view of the disk structure. The overall color profile suggests a mixed stellar population, with both older, redder stars concentrated in the bulge and younger, bluer stars populating the spiral arms. The galaxy exhibits some degree of rotational symmetry as expected for a spiral galaxy, and does not appear to be strongly elliptical.
