The galaxy appears as a centrally concentrated, relatively smooth object with a slightly elliptical morphology. The color profile is dominated by a broad, moderately bright yellowish-white hue suggesting a stellar population that is not intensely young but also not absent of star formation. There is a subtle bluing in the outer regions of the galaxy, suggestive of ongoing, though perhaps relatively low levels of star formation compared to more actively star-forming galaxies. Faint features are suggestive of possible tidal disturbances or asymmetries in the outer halo, potentially indicative of minor mergers.
