The galaxy presents as a flattened, elliptical object with a dominant central bulge. It exhibits a smooth light distribution, with a gradual decrease in brightness from the core outwards. While the galaxy appears mostly smooth, there are hints of faint, diffuse features or a possible disk structure oriented nearly edge-on, but further investigation and higher resolution imaging would be needed to confirm this. The color of the galaxy suggests an older stellar population with a yellowish-orange hue, indicating a lack of significant ongoing star formation. There may be minor disturbances present, possibly due to minor gravitational interactions, but nothing significant or noticeable. There appears to be no major merger event.
