The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated central bulge with a diffuse halo extending outwards. The galaxy is moderately bright, displaying a yellowish hue. There is a slight elongation in its shape, suggesting a possible deviation from a perfectly spherical morphology. No prominent spiral arms or distinct features are visible, indicating a lack of significant recent star formation activity. The overall appearance suggests a well-evolved system dominated by older stellar populations. Evidence of any ongoing merger activity or significant tidal disturbances is absent.
