The galaxy presents as an elliptical type, displaying a smooth, featureless morphology. Its shape appears moderately flattened, exhibiting an intermediate ellipticity between a circular and elongated form. The central region shows a concentrated brightness, indicating a significant stellar density, while the light gradually diminishes outwards toward the edges of the galaxy. There is little evidence of spiral arms or dust lanes; the overall color appears yellowish, suggesting an older stellar population. There is no distinct evidence of any major ongoing mergers or significant tidal disturbances.
