The galaxy presents as a diffuse, centrally concentrated object. Its overall form is spheroid-like, with a significant fraction of its light emanating from a relatively smooth and rounded core. The color suggests an older stellar population, with a dominant reddish-yellow hue, indicating fewer young, hot stars and more evolved, cooler stars. There appears to be evidence of an interaction with another galaxy, which is observed as a faint, diffuse object. There is no clearly defined spiral structure or prominent dust lanes visible. Given its redshift, it is a galaxy located at a substantial distance from us.
