This galaxy appears to be a relatively smooth, elliptical galaxy. The light profile suggests a high degree of central concentration, with a bright core and a gradual decrease in luminosity outwards. The galaxy is generally round in appearance with a hint of a flattened disk, and appears to be undisturbed, showing no strong signs of recent or ongoing major mergers. There may be a slight disturbance or a faint tidal feature, as evidenced by the small degree of uneven light distribution, indicating potential past minor interactions with smaller galaxies. It exhibits a yellow hue, hinting at an older stellar population. There is evidence of some ongoing, but relatively low level of star formation activity. The size of the galaxy is moderately extended, corresponding to a mass on the order of a large galaxy.
