The galaxy presents a primarily smooth morphology, appearing as a single, relatively cohesive structure. The central region exhibits a bright, concentrated core, likely indicative of a high stellar density, potentially an active galactic nucleus. A slightly elongated distribution of light extends outwards from the core, suggesting a flattened or disk-like structure.

The color gradient suggests a mix of stellar populations. The yellowish-white hue of the core possibly reflects an older, more evolved stellar population, while the slightly bluer, less concentrated region towards the outer edges indicates the presence of younger, hotter stars, suggesting ongoing or recent star formation.

Overall, the galaxy appears to be an intermediate mass system exhibiting characteristics of both elliptical and spiral galaxies, although the dominance of the smooth component suggests a higher likelihood for classification as an elliptical galaxy. There's a hint of a disturbance or an irregularity in the overall shape, potentially indicating a past interaction or merger event.
