The galaxy presents as a somewhat centrally concentrated object, exhibiting a smooth morphology. The color profile appears relatively uniform across the galaxy, suggesting a lack of significant color gradients. The light is concentrated to the center, with a generally round shape. There are no immediately obvious signs of spiral arm structures or a prominent disk. Faint structures around the edges indicate a possible merging event that has created tails or irregular shapes. The light from the galaxy is mostly in the green and red parts of the spectrum, implying some moderate star formation.
