The galaxy appears to be an elliptical galaxy, with a spheroidal morphology dominating its structure. It exhibits a smooth, featureless appearance, lacking prominent spiral arms or a well-defined disk. The central region displays a concentrated luminosity profile, indicative of a bulge component likely populated by older stars. The outer regions show a gradual decrease in luminosity, extending into a faint halo. The color gradient suggests a possible transition from a redder, older stellar population in the center to a slightly bluer, younger population in the outer regions. Overall, the galaxy presents a generally smooth, elliptical shape with a high degree of central concentration. There is a slight possibility of some minor disturbance occurring in the surrounding area. This galaxy is likely relatively massive and has a moderate amount of star formation.
