The galaxy presents a smooth, elliptical morphology. It exhibits a bright, concentrated central bulge that gradually fades into an extended halo. The color profile suggests an older stellar population, with a dominant yellowish-red hue indicating a lack of significant recent star formation. There is no obvious spiral arm structure or dust lane visible. The galaxy appears relatively undisturbed, with no major signs of tidal interactions or mergers. Its overall structure is generally round, with only slight elongation noticeable.
