The galaxy presents as a concentrated, elliptical-like form. The central region exhibits a high degree of luminosity, suggesting a dense population of stars and/or an active galactic nucleus. The light from the galaxy shifts in color from the center outwards; it is more yellow in the center of the galaxy, shifting to a slight blue-ish hue at the edges. The galaxy shows little evidence of spiral arms or significant dust lanes. The outer edges of the galaxy appear somewhat diffuse, gradually fading into the background sky. The overall structure indicates an evolved system, likely with a relatively low rate of ongoing star formation.
