The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth morphology with a high degree of central concentration. Its overall shape appears slightly elongated, not perfectly spherical, trending toward an in-between state between round and cigar-shaped. The central region displays a yellowish hue, suggestive of an older stellar population and a low rate of current star formation. A lack of well-defined spiral arms or prominent dust lanes suggests a relative absence of ongoing star formation. There are some indications of minor disturbances or interactions.
