The galaxy presents as an elliptical-shaped object with a smooth, featureless morphology. It exhibits a concentrated central bulge, appearing brightest towards the core with a gradual decrease in luminosity towards the edges. The color profile is predominantly redder hues, suggestive of an older stellar population. The galaxy does not show any prominent spiral arm structures or dust lanes. Its elongated shape indicates a relatively high ellipticity. There is no visual evidence of any ongoing major merger activity or significant tidal disturbances; however, minor irregularities may be present. The overall appearance is consistent with that of a mature, relatively quiescent galaxy, likely experiencing a low rate of star formation. The estimated size indicates that it is neither a dwarf galaxy nor a particularly large galaxy.
