The galaxy appears to be a relatively smooth, elliptical or lenticular type galaxy, exhibiting a centrally concentrated bulge region with a gradual fading of luminosity towards its outer edges. There is a hint of a disk-like structure, but it is not clearly defined. The galaxy appears to be yellowish in color, suggesting an older stellar population. A slight blueish hue is observed on one side, which may indicate some minor star forming regions. The overall morphology suggests the galaxy is not undergoing any major mergers, though there might be some disturbances. The apparent roundness indicates it is more circular than elongated.
