The galaxy presents as an elliptical morphology. The central region exhibits a high surface brightness, with a yellowish hue, suggestive of an older stellar population. The light is relatively smooth and concentrated toward the center, with a notable decrease in brightness outwards. There is little visible dust or distinct spiral arm structure present. Faint diffuse light extends slightly outwards from the bright core, hinting at a more extended halo component, however, this is not well-resolved. There is very little sign of disturbance or asymmetry, suggesting that it is relatively settled gravitationally. The galaxy is not perfectly circular, with an aspect ratio indicating a somewhat flattened elliptical form. No signs of tidal features or ongoing mergers are apparent.
