The galaxy presents a smooth, elliptical morphology. It is elongated in shape, appearing somewhat cigar-like. The core exhibits a brighter, concentrated region. The color gradient suggests an older stellar population dominates the galaxy's composition. There is minimal evidence of spiral arms or significant dust lanes. No major mergers appear to be occurring. The galaxy shows no clear signs of active star formation and is a fairly relaxed system. The estimated size is approximately 6 kpc across.
