The galaxy presents a mostly smooth morphology, with a hint of disk-like structure. The core appears fairly concentrated, exhibiting a brighter, somewhat reddish hue. The outer regions show a more diffuse, bluish glow. The galaxy's shape appears somewhat elongated, but is closer to round than cigar-shaped. There seems to be a minor disturbance within the galaxy, perhaps indicating a weak interaction or an internal dynamic process. Based on the bluer colors in the outskirts and relatively high star formation rate, there is evidence of ongoing star formation activity, despite the dominant smoother, rounder morphology associated with more quiescent galaxies.
