The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge with a gradual decrease in luminosity towards the outer regions. The dominant color appears yellowish-orange, indicative of an older stellar population. The galaxy does not show any prominent spiral arms or significant dust lanes. It appears fairly isolated and not currently undergoing a major merger event, though a slight asymmetry or minor disturbance cannot be entirely ruled out. The shape is generally round, with little elongation.
