The galaxy appears as a slightly elongated, diffuse object with a yellowish hue. Its morphology suggests a possible elliptical galaxy, although a disk component cannot be entirely ruled out due to the limited resolution. The light distribution appears relatively smooth with a gradual decrease in intensity from the center outwards. There are no immediately obvious signs of spiral arms or significant dust lanes. Some evidence of a minor disturbance is possible. The galaxy shows some sign of star formation.
