The galaxy presents a smooth, elliptical morphology. The light distribution appears centrally concentrated, exhibiting a bright, relatively small core. Moving outward, the light gradually fades, with a slight elongation. No distinct spiral arms or other defined structures such as dust lanes are discernible. The overall color is yellowish-white, suggesting an older stellar population with minimal ongoing star formation. There is a faint blue hue on the edges of the galaxy. There is no evidence of major mergers or tidal disturbances. The galaxy appears to be relatively isolated.
