The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. A subtle color gradient is observable, transitioning from a more yellowish-white hue in the central region to a bluer tint in the outer regions. The galaxy appears to be fairly compact, its light profile fading gradually into the background sky. There is slight indication of distortion, possibly suggestive of a minor interaction or disturbance in its recent history. The overall light distribution suggests a population of older stars in the central bulge, with a younger population contributing to the bluer color in the outskirts. No prominent spiral arm structures or distinct dust lanes are visible.
