The galaxy appears as a centrally concentrated object with a generally smooth morphology. The core displays a yellowish-orange hue, potentially indicating an older stellar population with fewer young, blue stars and a dominance of redder giants and dwarfs. The surrounding halo exhibits a gradual fading in intensity, with hints of a slightly elongated, disklike structure, although distinct spiral arms or prominent features are not readily discernible. There may be some minor disturbances present. The overall visual impression suggests an evolved galaxy transitioning toward a redder color profile.
