The galaxy appears to be a relatively compact, elliptical system. Its morphology is dominated by a smooth, spheroidal component, with a noticeable concentration of light towards the center. The color profile suggests an older stellar population, with a yellowish-orange hue dominating the central region. There is a subtle color gradient, transitioning to slightly bluer tones in the outer regions. Evidence of a disk component or spiral arms is not readily apparent in this image, but it is possible there is a smooth disk. The galaxy does not show any obvious signs of major mergers or significant tidal disturbances. There may be evidence of a close partner or recent minor merger.