The galaxy presents a largely smooth morphology. The central region exhibits a high degree of luminosity, appearing almost uniformly bright. The light from the galaxy is spread out in a near circular shape. There appears to be little evidence of defined spiral arm structures, although there may be some faint distortions within the surrounding regions. There is no apparent ongoing major merger activity, such as tidal tails or clear double nuclei, but it appears to have some minor disturbances from another galaxy.
