This galaxy appears to be a relatively smooth, elliptical-type galaxy. It exhibits a centrally concentrated bulge that dominates its overall structure. The color profile suggests a higher concentration of older stellar populations, giving it a yellowish hue, especially within the core. There is minimal evidence of spiral arm structure or significant dust lanes. The galaxy's light profile appears fairly uniform, with the light intensity decreasing gradually from the center outwards. Overall, the galaxy presents a symmetrical and well-defined shape, indicating a dynamically relaxed system. There are no obvious signs of tidal disturbances or ongoing major mergers. However, the system might be exhibiting low levels of star formation.
