The galaxy appears as a roughly elliptical-shaped object, exhibiting a smooth light distribution. The color profile suggests a dominant population of older stars, giving it a reddish-yellow hue. There is little indication of spiral arm structure or significant dust lanes, implying a relatively quiescent state of star formation. There is no obvious sign of any major ongoing merger activity, though a faint asymmetry in the outer regions could point to minor gravitational interactions. Overall, the morphology indicates a relatively evolved galaxy with a substantial stellar mass.
