The galaxy presents a smooth, elliptical morphology, lacking prominent spiral arms or a well-defined disk structure. It appears largely featureless, with a high degree of central concentration and a gradual decline in surface brightness towards its outer regions. The galaxy exhibits a relatively uniform color distribution, with a slightly reddish hue, indicative of an older stellar population and lower ongoing star formation. There is no visual evidence of any significant interaction with other galaxies, such as tidal tails or distorted morphology, but there is possibly a very minor disturbance. The general appearance suggests a mature galaxy, potentially an elliptical or lenticular type, at a moderate distance, based on its apparent size and faintness. The light emitted is indicative of a mass of around 10^10 solar masses.
