The galaxy presents a largely smooth, elliptical morphology. It appears nearly round in projection with a slightly elongated shape. There is a high degree of central concentration of light, diminishing outwards from the core. Some minor disturbances may exist in the form of faint, diffuse features. The overall color is yellowish, suggesting a relatively older stellar population. This is consistent with a lower rate of star formation. The galaxy appears to be relatively isolated, with no major signs of ongoing or recent merger activity.
