The galaxy appears to be a relatively smooth, elliptical-like system. There is a bright, concentrated central bulge, exhibiting a yellowish hue, suggesting an older stellar population. The outer regions display a bluer color, indicating the presence of younger, hotter stars, potentially indicative of ongoing, although subdued, star formation. The galaxy's overall morphology leans towards an elliptical type but there is evidence of a faint disk-like structure. The roundness is somewhere between round and cigar-shaped. There are no obvious signs of major mergers or strong tidal disturbances. The galaxy shows only minor signs of disturbance.
