The galaxy presents as a largely featureless elliptical morphology. The light is centrally concentrated, exhibiting a smooth radial gradient in surface brightness. The core appears to be a yellow/orange hue, possibly indicating an older stellar population. Progressing outward from the core, a subtle shift towards bluer wavelengths is apparent. There is no discernible spiral arm structure or prominent dust lane. The isophotes display a generally rounded shape, with only a minor deviation from perfect circularity. There does not appear to be any evidence of active galactic nuclei activity or strong tidal interactions. Based on the color and overall morphology, star formation rates are expected to be relatively low.
