The galaxy presents a generally smooth, elliptical morphology, showing a significant degree of central concentration. The light profile appears regular with a smooth fall-off from the center. Its core displays a yellowish hue, suggesting a stellar population of older, redder stars. There is a noticeable, lower-intensity, reddish glow emanating from other spots within the galaxy, which could indicate older stellar populations or dust obscuration. The galaxy does not exhibit a well-defined spiral arm structure. The overall structure of this galaxy does not show major disturbances or ongoing mergers.
