The galaxy presents a smooth, elliptical morphology, with a noticeable central bulge. The light distribution appears relatively even and diffuse, with no distinct spiral arms or strong dust lanes visible. The galaxy exhibits a color gradient, shifting from a more yellow/red hue at the core to slightly bluer colors in the outer regions. It displays an elongated shape, appearing more "in between" rather than perfectly round or highly elongated. There are no obvious signs of major interactions or mergers, although subtle irregularities might indicate minor past disturbances. Overall, the galaxy appears to be a relatively evolved system, potentially with suppressed star formation activity and a dominant population of older stars within the central region.
