The galaxy appears to be an elliptical or lenticular type. It exhibits a generally smooth morphology with little apparent substructure such as spiral arms or dust lanes. The central region displays a higher concentration of luminosity, fading gradually towards the outer edges. The overall shape is largely circular, with only a slight deviation from perfect roundness. There is no obvious evidence of ongoing major merging activity or significant tidal disturbances in its immediate vicinity, although some minor disturbances cannot be ruled out. The galaxy presents a reddish color, suggesting an older stellar population and relatively low current star formation activity. Based on its color, this galaxy is composed of older stars and is relatively massive.
