The galaxy presents as a smooth, elliptical structure. Its core is bright and concentrated, exhibiting a yellow-white hue indicative of an older stellar population. The radial light profile suggests a gradual decline in luminosity from the center outwards. There is a slight elongation but the galaxy is largely round in appearance. The overall color is reddish, implying a lack of significant ongoing star formation. Subtle irregularities, possibly minor disturbances, are suggested by the asymmetric distribution of light. There is no clear evidence of spiral arms or a distinct disk component.
