The galaxy presents as a relatively smooth, centrally concentrated object. There is a slight elongation, but overall appears fairly round. The central region exhibits a bright, yellowish core. The outer regions of the galaxy display a more diffuse, bluish halo, suggesting a population of younger, hotter stars in these areas. There is a faint hint of a possible tidal interaction or minor disturbance in the outskirts, possibly due to a smaller, nearby companion galaxy. Star formation is likely occurring, albeit at a moderate rate.
