The galaxy presents as a slightly elongated, lenticular-shaped object. It exhibits a smooth, largely featureless structure, suggesting a relatively evolved system. The light distribution is centrally concentrated with a gradual falloff in intensity towards the edges, indicative of a centrally dominant bulge. No distinct spiral arm structures or dust lanes are discernible, furthering the classification as a lenticular galaxy. The light from this galaxy is primarily expressed in the redder wavelengths with hints of green and blue, suggesting an older stellar population with subdued levels of on-going star formation. There appears to be no major disturbance in the galaxy's form, though a minor disturbance cannot be ruled out given the image resolution.
