The galaxy appears to be a relatively smooth, elliptical-like structure. The central region exhibits a bright, concentrated luminosity, suggesting a dense stellar population or possibly an active galactic nucleus. The galaxy displays a noticeable elongation, with the major axis extending more prominently than the minor axis. A subtle color gradient is observed, transitioning from a yellowish-orange hue in the core to a slightly bluer tint in the outer regions. No distinct spiral arms or significant dust lanes are visible, implying a lack of active star formation in the main body of the galaxy. There are no signs of any major mergers occurring, however, there may be some minor disturbance in the galaxy's overall form.
