This galaxy appears to be a relatively smooth, elliptical-like structure. The core is noticeably brighter and more concentrated, suggesting a higher density of stars towards the center. The galaxy exhibits an elongated shape, more cigar-shaped than perfectly round. There is no indication of major merging events, although a slight asymmetry in the outer regions might hint at minor gravitational interactions. The galaxy exhibits a yellowish-orange hue, implying an older stellar population with lower levels of ongoing star formation. We do not see any spiral arms or prominent dust lanes.
