The galaxy presents as an elliptical-like morphology, exhibiting a relatively smooth and diffuse structure. There are no discernible spiral arms or significant dust lanes apparent in this image. The galaxy displays a central concentration of light that gradually fades outwards, suggesting a higher stellar density in the galactic nucleus. The color profile indicates a generally older stellar population, with a yellowish-orange hue dominating the central region, possibly indicating a higher proportion of evolved stars. Faint blue regions are visible along the edge of the galaxy. The overall shape appears to be slightly elongated. The general appearance suggests minimal ongoing star formation. There are no obvious signs of major tidal disturbances or ongoing mergers in this image, though there may be signs of minor disturbances.
