The galaxy presents a flattened, elliptical morphology. It is relatively compact. A central, bright core region is observed, exhibiting a cyan hue, possibly indicative of intense star formation activity or an active galactic nucleus. Surrounding this core is a fainter, diffuse halo, which graduates from cyan to blue. There is weak evidence of faint, reddish regions located within the galaxy’s outer boundaries. There is no clear spiral arm structure or bar feature observed. Based on its light profile, it is likely a relatively smooth galaxy. Marginal evidence indicates that it may be undergoing minor disturbance.
