This galaxy exhibits a predominantly smooth morphology, with a high degree of central concentration. The light distribution suggests a spheroid-dominated system, likely an elliptical galaxy or an early-type spiral with a significant bulge component. There is a subtle hint of disk structure, but it is not prominent. The color gradient indicates a population of older stars, predominantly reddish in hue, especially towards the galactic core. The light appears less intense in the outer regions. There are also signs of two reddish objects, which are potentially merging features or minor disturbances in the galaxy's overall form. There do not appear to be distinct spiral arms or strong star-forming regions visible, which is consistent with a more quiescent galaxy.
