The galaxy presents as a smooth, centrally concentrated object with a generally elliptical morphology. The galaxy exhibits a yellow-orange hue, indicating an older stellar population with a minimal amount of recent or ongoing star formation. There is little to no discernible spiral arm structure or dust lane obscuration. There are no obvious signs of tidal tails or distorted morphology suggestive of any recent or ongoing major merger events. However, there appears to be minor disturbance to the main body. The object is relatively round in appearance, with only slight ellipticity.
