The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated, luminous core that gradually fades into a more diffuse outer region. The color gradient suggests an older stellar population, with the central regions appearing more yellow and the outer regions trending towards red. There is no discernable spiral arm structure or dust lanes. The galaxy appears relatively isolated and undisturbed, without obvious signs of tidal interactions or ongoing mergers, though some minor irregularity in the outskirts is observed. Overall, the galaxy appears as a quiescent, passively evolving system.
