The galaxy appears to be a relatively smooth, elliptical-type galaxy. Its light profile is concentrated toward the center, forming a bright nucleus, with the luminosity gradually decreasing outwards. The overall shape appears somewhat rounded. There is no clear indication of spiral arms or a prominent disk structure within the observable light. A slight color gradient is observed, with the central region appearing bluer and the outer regions tending towards redder hues. This indicates potential differences in stellar populations, with younger, hotter stars concentrated in the center and older, cooler stars more prevalent in the outer areas.
