The galaxy presents as a relatively smooth, centrally concentrated object. It has a generally elliptical morphology with high roundness. No distinct spiral arm structures or prominent dust lanes are visible. The core exhibits a somewhat brighter, diffuse glow, gradually fading towards the outer edges. There appears to be some minor internal disturbance, however the shape is largely undisturbed. The overall color is slightly bluer in the core, transitioning towards a redder hue in the outer regions. This suggests a potential difference in stellar populations, with younger, bluer stars concentrated near the galactic center and older, redder stars dominating the periphery.
