The galaxy presents a generally smooth, elliptical morphology. A bright, concentrated core region is observed, with diffuse light extending outwards. The color gradient suggests a relatively older stellar population, with a bluer halo around the core. There is no distinct spiral arm structure visible, nor is there any obvious dust lane obscuration. The overall impression is of a relatively quiescent system, without any major ongoing merger events or significant star formation. The galaxy appears to be relatively isolated, without any obvious nearby companions influencing its morphology through tidal interactions. The elongation suggests it is not perfectly spherical.