The galaxy appears to be a relatively large, elongated system. Its light is dominated by reddish-yellow hues, indicative of an older stellar population and/or significant dust obscuration. The galaxy's overall structure lacks defined spiral arms or a prominent disk. The morphology suggests it is likely an elliptical or lenticular galaxy, possibly viewed at an angle. There's a faint suggestion of some disturbance in the main body of the galaxy, but a merger event appears unlikely. Overall, the galaxy presents as a fairly smooth and undisturbed system.
