The galaxy presents as an elliptical morphology, displaying a smooth, centralized luminosity profile with a notable lack of distinct spiral arm structures. The light distribution suggests a concentration of older stellar populations. It exhibits a warm color with a slight reddish hue, indicating a relatively low rate of recent star formation. The galaxy has a somewhat elongated shape, not perfectly circular but tending toward oval. No signs of strong gravitational disturbance, such as tidal tails or obvious mergers, are apparent in the visual data. The galaxy appears to be an isolated system without any nearby companions.
