The galaxy appears to be a relatively smooth, round, elliptical galaxy. There are no visible spiral arms or a distinct disk. There is a high central concentration of light, indicative of a prominent bulge. A slight color gradient can be observed, with the central region displaying a subtly redder hue that fades outwards into a more greenish color, perhaps implying an older stellar population at the core. The galaxy exhibits no obvious signs of ongoing merging or tidal disturbances. The estimated size of the galaxy is fairly compact. Overall, the galaxy presents as a relaxed system with a dominant spheroidal component.
