The galaxy presents as a centrally concentrated system with a largely smooth morphology. It appears elliptical in shape, exhibiting a high degree of radial symmetry, with the ratio of major to minor axis close to unity, suggesting it is close to round. There is a noticeable color gradient, with the central region appearing redder compared to the outer regions, which have a relatively bluer hue. The absence of clearly defined spiral arms or prominent dust lanes indicates a lack of significant ongoing star formation. There is no obvious evidence of major mergers or tidal disturbances, although there is a hint of minor asymmetry, which suggests the possibility of minor gravitational interactions in its past.
