The galaxy presents as a moderately luminous object, exhibiting a concentrated central bulge region. It is a relatively smooth structured galaxy, appearing largely elliptical in shape, though with some slight irregularities that may indicate a weak disk or interaction. The galactic core exhibits a slightly yellower hue than the surrounding halo, potentially indicating an older stellar population residing in the center. There are very faint indications of a blueish tinge in the outer edges of the galaxy. This could indicate a low level of ongoing star formation. No spiral arm structure is clearly visible, but some slight irregularities could indicate minor disturbances. Based on its moderate redshift, it exists at a significant distance. 
