The galaxy presents a generally smooth, elliptical morphology. Its light is concentrated towards the center, exhibiting a high degree of central luminosity. The galaxy is quite round and shows no apparent features, such as spiral arms or a prominent disk. There is no evidence of recent or ongoing major mergers or tidal disturbances. The color profile is relatively uniform, with a slight reddish hue indicating an older stellar population and low star formation rate. Given its size and observed color, it likely contains a significant population of evolved stars.
