The galaxy presents as an elliptical morphology, exhibiting a largely smooth and concentrated light profile. The color appears to be relatively uniform across the galaxy, with a slightly yellowish-orange hue indicating an older stellar population and lower levels of current star formation. There is no obvious spiral arm structure or dust lane obscuration apparent in the image. The galaxy has an apparent size of a few arcseconds, implying a physical diameter on the order of several kiloparsecs, given the approximate redshift. There are no obvious signs of a major ongoing merger or strong tidal features suggesting recent interactions, though there is a hint of a faint disturbance. The concentration of light towards the center of the galaxy suggests the presence of a supermassive black hole.
