The galaxy appears as a roughly elliptical, diffuse object with a yellow-orange hue, indicative of an older stellar population. The morphology is predominantly smooth with a slight elongation, suggesting it may be an elliptical galaxy or a lenticular galaxy viewed at an angle. There is no visible spiral structure or distinct disk component. Minor irregularities hint at possible gravitational interactions or recent accretion events, though no significant merger signatures are evident. The galaxy's relatively compact size, along with its color, implies a moderate level of star formation, potentially residing in a state of quenching.
