The galaxy appears as a largely featureless, concentrated object. It exhibits a generally elliptical morphology, with a high degree of roundness, with a smooth light distribution that decreases in intensity with distance from the galactic center. No distinct spiral arm structures or bar features are discernible in the image. There is little evidence of ongoing major mergers or tidal disturbances. The overall color index suggests the presence of an older stellar population. The galaxy has a moderate luminosity. Considering its overall appearance, it can be classified as an elliptical galaxy.