The galaxy presents as a singular, relatively smooth object. It appears to be elliptical in shape, with a high degree of central concentration, the light is strongly concentrated towards the center, which fades gradually toward the edges. The core of the galaxy exhibits a yellowish hue, suggesting an older stellar population. The outer regions exhibit a slightly bluer tint, which is most likely attributed to patches of younger stars. There's no discernible spiral arm structure or bar feature visible. There is some marginal distortion in the halo of the galaxy, which may be evidence of past or ongoing minor gravitational interactions. Overall, the galaxy appears to be a relatively massive, evolved system with a modest amount of recent star formation.
