The galaxy appears as a smooth, elliptical object. Its light profile shows a concentrated central bulge that gradually fades into the outer regions. The galaxy exhibits a color gradient, with a yellowish-white core transitioning to redder hues in the outer parts, possibly indicating a decrease in younger stellar populations away from the center. The overall shape suggests a galaxy that is neither perfectly spherical nor strongly disk-like but somewhere in between. There is no clear evidence of spiral arms, rings, or significant dust lanes. The galaxy is likely undergoing low levels of star formation. There is also little evidence of any major merging events or disturbances in its structure.
