The galaxy presents as a largely smooth, elliptical-like structure. Its light is concentrated towards the center, indicating a dense galactic nucleus. The color is primarily a yellowish-orange hue, suggestive of an older stellar population. There are only hints of spiral arm structures. No significant dust lanes or active star-forming regions are readily apparent. The galaxy appears fairly isolated, without obvious signs of recent or ongoing major mergers or tidal disturbances, though there may be a minor disturbance. Its shape is generally rounded. The overall morphology suggests a relatively evolved system, potentially a lenticular galaxy transitioning from spiral to elliptical.
