The galaxy presents as a spiral type, with a distinct disk and a moderately sized bulge. Spiral arms are clearly visible, exhibiting a relatively tight winding pattern. A bar structure appears to be present within the central region of the galaxy, possibly of moderate strength. The bulge appears yellow-ish, possibly indicating a population of older stars, while bluer hues are observed within the disk, particularly along the spiral arms. The spiral arms are somewhat flocculent in nature, exhibiting a discernible two-armed structure. No obvious signs of major merging activity or significant morphological disturbance are apparent; however, some minor irregularities could suggest past interactions. The galaxy is likely observed at a small inclination to our line of sight, as evidenced by the clear visibility of both the bulge and disk components.
