The galaxy presents as a centrally concentrated object, exhibiting a smooth, elliptical morphology. The core region displays a bright, yellowish hue, suggesting a significant population of older stars. The outer regions of the galaxy appear more diffuse and slightly redder in color, possibly indicating the presence of some dust or a population of cooler, redder stars. There's a subtle suggestion of flattening, though the galaxy appears largely spheroidal. There is no evidence of spiral arm structure or significant star formation regions discernible.
