The galaxy exhibits a smooth, elliptical morphology with a concentrated central bulge. The primary color is a yellowish-white, suggesting an older stellar population dominating the light output. There is little evidence of spiral arm structure or significant dust lanes. The overall shape appears somewhat rounded, although a subtle deviation from perfect circularity might indicate a slight elongation. There might be a very faint tidal tail, but this is within the margin of noise and could be a disturbance rather than a merging event. The light distribution appears relatively even with minimal signs of active star formation.