The galaxy presents as a singular, moderately luminous object with a concentrated central region. The core exhibits a yellowish-orange hue, which potentially indicates an older stellar population. The outer regions display a faint, diffuse halo. The shape appears to be largely smooth and elliptical, with a suggestion of a slight disk structure. There is no evident spiral arm structure or prominent dust lanes visible in the image. The morphology indicates this galaxy has a red shift of approximately 0.201926. There is no evidence of ongoing major merger events.
