The galaxy presents a smooth, elliptical morphology. It exhibits a concentrated central bulge that appears yellowish-orange in color, suggesting an older stellar population. The overall shape is elongated, with a cigar-like appearance. There are hints of a disk component, but it is not well-defined. No significant signs of ongoing mergers or tidal disturbances are apparent in the image. The galaxy's outer regions fade gradually, and the color shifts to slightly bluer hues, possibly indicating the presence of some younger stars in the outskirts, however, star formation appears to be quite low. The galaxy seems relatively isolated.
