The galaxy appears as a centrally concentrated, elliptical-like structure. It exhibits a relatively smooth, featureless morphology, lacking any distinct spiral arms or a prominent central bar. There is no evidence of any major tidal disturbances, such as extended plumes or distorted shapes, indicating it is likely not currently undergoing a major merger event, though a minor disturbance is possible. The galaxy presents a moderate red color index, hinting at a stellar population that is somewhat older and less actively forming stars. The roundness appears in between that of a circle and an ellipse. Overall, this galaxy appears to be a relatively isolated, moderately massive system with a suppressed rate of star formation, consistent with an early-type galaxy transitioning towards a more quiescent state.
