The galaxy presents as a relatively smooth, elliptical structure. It exhibits a distinct elongated shape, appearing cigar-shaped. There's a bright, concentrated central region that likely corresponds to the galactic nucleus. The color gradient suggests a higher concentration of older stellar populations in the core, indicated by the yellowish hue, gradually transitioning to bluer colors in the outer regions of the disk, indicating younger, star-forming regions. There is no evidence of major disturbances or ongoing merging events. There is subtle evidence of spiral arms, potentially flocculent. The galaxy exhibits a moderate amount of star formation activity.
