The galaxy appears to be a relatively smooth, elliptical type. It exhibits a centrally concentrated luminosity profile, with the brightest region located at the core. There is a slight elongation to the galaxy's shape, deviating somewhat from perfect circularity, appearing more rounded than cigar-shaped. There is a lack of significant features such as spiral arms or prominent dust lanes, suggesting a classification towards the early end of the Hubble sequence. Overall, the galaxy seems to be relatively undisturbed, showing no obvious signs of major interactions or merging events. The color of the galaxy indicates an older stellar population and minimal on-going star formation.
