The galaxy presents an overall elliptical morphology, exhibiting a smooth and largely featureless structure. There is a concentrated central bulge with a reddish hue. The galaxy displays an intermediate ellipticity, not perfectly spherical but also not highly elongated. A faint, diffuse disk component is possibly present, indicated by a subtle extension of light along the horizontal axis, yet it lacks clearly defined spiral arms or distinct dust lanes. Color gradients suggest some variation in stellar populations or dust content across the galaxy. The central bulge appears to host older stars, while the faint disk may contain younger stars. The galaxy does not show any obvious signs of major interactions or mergers, although some subtle disturbances could be present in the outer regions.