The galaxy presents a well-defined disk structure, viewed at a slight angle, close to face-on. Spiral arms are discernible, exhibiting a somewhat flocculent morphology. A central bulge is apparent, possessing a moderate size relative to the overall galactic disk. The color profile suggests the presence of both younger, bluer stellar populations within the spiral arms and an older, redder population concentrated in the bulge. There is no immediate evidence of strong tidal disturbances or a major merger event, although subtle asymmetries within the spiral arm structure cannot be ruled out as indicative of minor interactions. A weak bar structure might be present, though its definition is somewhat obscured by the arm morphology. The galaxy exhibits a notable degree of internal structure, indicating active or recent star formation processes. The relative smoothness of some regions of the disk suggests the presence of more quiescent stellar populations as well.
