The galaxy presents as a relatively smooth, elliptical morphology. The light is concentrated toward the center, exhibiting a bright core that gradually diffuses outwards. The overall color profile appears to be on the redder end of the spectrum, suggesting an older stellar population. The galaxy exhibits a largely symmetrical structure without any prominent spiral arms or irregular features. There are no signs of ongoing major mergers or significant tidal disturbances. The galaxy seems to be well-formed and relatively undisturbed.
