The galaxy presents a generally smooth and centrally concentrated morphology. It exhibits a nearly round shape, with a slight elongation barely perceptible. The central region is significantly brighter than the outer regions, suggesting a substantial stellar bulge or a very active galactic nucleus. The galaxy exhibits a color gradient, with the core showing a slightly bluer hue that gradually transitions to redder colors as it moves towards the outer regions. This suggests a population of younger, hotter stars in the central region, with older, cooler stars dominating the outer areas. No clear spiral arm structures or distinct dust lanes are visible, indicating a relatively undisturbed morphology. There is no significant evidence of recent or ongoing merger activity. The galaxy appears relatively isolated in this field of view.
