The galaxy appears to be a relatively smooth, elliptical type, with a high degree of roundness. The central region exhibits a bright, concentrated luminosity, fading gradually outwards. There is some indication of a faint, disk-like structure or possibly a tidal feature extending from the main body, characterized by a slightly bluer tint, which may indicate an area of recent or ongoing star formation, though it could be a foreground or background object along the line of sight. The galaxy doesn't present any obvious signs of major mergers or significant disturbances. Overall, the galaxy appears to be relatively quiescent, potentially with a low rate of star formation.
