This galaxy appears to be an elliptical galaxy with a smooth, diffuse morphology. Its light distribution suggests a relatively homogeneous stellar population. The galaxy is elongated, with a roughly cigar-shaped profile. There is a prominent central bulge that decreases smoothly in brightness. There is evidence of some disk-like features present, however the prominent bulge is more apparent. There is no clear evidence of spiral arms or active star formation within the visible region. There are no obvious signs of ongoing or recent major mergers or strong tidal disturbances and appears relatively isolated.