The galaxy exhibits a generally elliptical morphology, appearing somewhat elongated in shape. The light distribution suggests a smooth profile, with no immediately obvious spiral arm structures or prominent dust lanes. The core of the galaxy displays a moderate concentration of light, fading gradually outwards. Color gradients are subtle, with the central region appearing slightly bluer than the outer regions, which could indicate ongoing, but subdued, star formation activity. There is no evidence of tidal tails or other clear signs of a recent major merger event, although some minor irregularities in the outer isophotes might suggest past interactions. Overall, the galaxy appears to be a relatively undisturbed system, transitioning from more active star formation in the recent past.
