The galaxy appears as a centrally concentrated, relatively smooth object. The core exhibits a bright, yellowish-orange hue, suggesting an older stellar population. There is a slight elongation, hinting at a possible elliptical morphology, though a disk cannot be entirely ruled out. Fainter, greenish-blue extensions are observed surrounding the central bulge, potentially indicative of some star formation, albeit at a low rate. There are no obvious signs of a major ongoing merger or significant tidal disturbances. The overall morphology is generally undisturbed, likely an isolated system with an estimated stellar mass towards the higher end.
