The galaxy presents as an elliptical morphology, appearing as a smooth, concentrated object with a notable absence of distinct spiral arms or prominent disk structures. The light distribution is relatively uniform, suggesting a well-mixed stellar population. The color gradient transitions from a yellowish central region outwards to redder peripheries, which indicates an aging stellar population in the outer regions of the galaxy. There is a suggestion of minor tidal disturbances. The galaxy has a moderate size, it's luminosity indicates a relatively massive galaxy. The estimated star formation rate suggests the galaxy has been quenching in the recent past. 
