The galaxy presents an elliptical morphology, appearing smooth and relatively featureless in this imaging. The light profile is centrally concentrated with a radial fall-off, typical of elliptical galaxies. The core region exhibits a yellowish hue, potentially indicative of an older stellar population. The isophotes appear mostly regular, with a slight elongation, suggesting it is not perfectly spherical. There is no readily apparent spiral structure or dust lanes present. The outer regions show a faint, diffuse glow, gradually blending into the background sky. The lack of discernible features suggests a dynamically relaxed system. The light distribution indicates minimal ongoing star formation activity.
