The galaxy presents as a relatively compact structure. Its overall appearance is somewhat smooth, with a centrally concentrated luminosity profile. There is evidence of some bluer star formation regions scattered throughout the galaxy, especially near the center and along its periphery, though this is not the dominant feature. There's a slight hint of disurbance to the galaxy’s overall morphology, not overwhelmingly pronounced, but subtle ripples or asymmetries can be seen. The galaxy’s color index suggests the presence of both older stellar populations responsible for the more reddish hues in the central regions, and younger, bluer stars in the star-forming areas. It does not appear to be undergoing a major merger, but may have experienced minor interaction based on the subtle morphological disturbances.
