The galaxy presents a predominantly smooth, elliptical morphology. It exhibits a high degree of central concentration, with light intensity decreasing gradually towards the outer regions. The color gradient suggests a relatively old stellar population, dominated by evolved stars. There is a slight elongation, deviating from a perfectly circular shape, hinting at possible past interactions or internal dynamics. Evidence of a faint tidal tail is not apparent. A slight disturbance can be seen on the right side of the galaxy, but is not thought to be a merger.
