The galaxy appears as a centrally concentrated, luminous spheroid. The core exhibits a yellowish-orange hue, suggesting an older stellar population and a dearth of ongoing star formation. Moving outwards from the core, the galaxy exhibits a slight decrease in surface brightness, transitioning to a more diffuse, greenish-yellow halo. There are no clear spiral arm structures or distinct features indicative of recent mergers or significant tidal disturbances. The overall morphology is relatively smooth, with a subtle elongation along a single axis. No prominent dust lanes are visible. The lack of blue light or bright knots of emission suggests that active star formation is not a dominant process within this system.
