The galaxy presents as a single, relatively well-defined object. It exhibits a morphology consistent with an elliptical galaxy. Its overall shape is largely round, showing minimal deviation from a circular form. The light distribution appears smooth and centrally concentrated, with a gradual decrease in surface brightness from the core outwards. No distinct spiral arms or prominent disk features are discernible. There is a faint suggestion of a tidal tail.

Evidence of significant ongoing mergers or major disturbances is not immediately apparent, though subtle irregularities could indicate minor gravitational interactions. The galaxy exhibits colors that indicate it may be composed primarily of older stellar populations.
