The galaxy presents as a relatively smooth, centrally concentrated object with an elliptical morphology. It exhibits a bright, compact core, suggesting a high stellar density in the central region. The galaxy's light profile fades gradually from the core outwards, showing no distinct spiral arms or prominent disk features. There are subtle color gradients, with the core appearing whiter and the outer regions showing a slightly redder hue. This could indicate a population of older, redder stars in the outskirts of the galaxy. No significant signs of tidal disturbances, merging activity, or active star formation regions are apparent in the image. The overall structure suggests a relaxed system that has undergone significant evolution.
