The galaxy presents a largely smooth and elliptical morphology. It appears relatively round in shape with no obvious spiral arm structures or a prominent disk. The central region displays a high concentration of light, suggesting a substantial bulge component. The overall color profile is predominantly yellow, implying an older stellar population. Some slight disturbance is visible in the galaxy's form, likely due to minor tidal interactions. There is no strong evidence of ongoing major mergers. The galaxy's smooth appearance suggests that star formation is relatively low.
