The galaxy presents as an elliptical morphology with a high degree of central concentration. The light profile appears smooth, exhibiting a largely featureless structure with no readily discernible spiral arms or bar. It is relatively luminous, suggesting a large stellar population, and appears to be in a relatively quiescent state regarding star formation. The galaxy has an intermediate axis ratio, exhibiting a shape that is neither perfectly spherical nor highly elongated. There are no obvious signs of tidal disturbances or ongoing mergers in the immediate vicinity, indicating that it may be relatively isolated.
