This galaxy appears to be a relatively bright, smooth object. It exhibits a concentrated central bulge, which graduates outward into a less defined disk. The overall morphology is elliptical or lenticular, appearing nearly round in shape. There are no obvious spiral arm structures visible; instead, a homogenous distribution of light is observed from the core to the outer regions. The color profile indicates a yellow hue, which suggests an older stellar population dominating its composition. There is no evidence of ongoing major mergers or significant tidal disturbances, though some minor asymmetries in the outer regions cannot be ruled out with absolute certainty from the present image quality. The object gives the impression of relative quiescence.
