The galaxy appears as a luminous, centrally concentrated object. Its overall morphology is generally smooth, lacking prominent spiral arms or strong bar features. There may be a very subtle disk component, though it's not definitive. The galaxy exhibits a yellow-orange hue, suggesting an older stellar population. The light is concentrated around the center of the galaxy, implying a large bulge, with what may be a small halo. There is no significant evidence of ongoing major merger activity or strong tidal disturbances in the image.