The galaxy appears to be a relatively smooth, elliptical type. It has a concentrated central bulge that exhibits a yellowish hue, likely indicating an older stellar population. The overall shape is mostly round, with only a slight elongation. There's a hint of bluer light in the outer regions, which might suggest the presence of some younger stars or ongoing, albeit weak, star formation. The galaxy shows no visible signs of any major disturbances or recent merger activity.
