The galaxy presents as a relatively smooth, centrally concentrated object. The overall morphology appears to be elliptical or lenticular, exhibiting a somewhat elongated, but not highly flattened, shape. A dominant central bulge is observed, characterized by a yellowish-orange hue, suggesting an older stellar population. Fainter, more diffuse blue light is seen surrounding a portion of the bulge, potentially indicating some ongoing star formation, albeit at a low rate. There may be minor disturbances present. It does not seem to be undergoing a major merger.
