The galaxy appears to be a relatively smooth, elliptical-like structure, exhibiting a radial gradient in surface brightness, with a bright, concentrated core that fades towards the edges. The core region shows a yellowish hue, suggesting an older stellar population. Surrounding the core is a broader, less defined halo that exhibits a slightly bluer color. This suggests the presence of a younger stellar population and potentially ongoing star formation within the galaxy, though the overall morphology is indicative of a galaxy dominated by older stars. There are no obvious signs of strong tidal interactions or major mergers, though minor irregularities or disturbances in the outer regions cannot be ruled out at this resolution. The overall shape appears close to circular, suggesting a relatively low degree of rotational support.
