The galaxy presents as a relatively smooth, rounded structure. Its light profile suggests a single, dominant component without obvious spiral arms or a prominent bar. There's a distinct central concentration of light that diminishes gradually towards the outer regions of the galaxy. The core appears quite bright and almost point-like, indicative of a possible active galactic nucleus or a dense stellar population. The color appears to be more yellow/red in the center, transitioning to green on the outer edges. Based on these characteristics, the galaxy might be an elliptical galaxy or a lenticular galaxy viewed face-on. Subtle irregularities or minor disturbances might be present in the galaxy's structure, but not significant enough to classify it as a major merger event.
