The galaxy presents as a centrally concentrated, relatively smooth object. The overall morphology appears elliptical, trending toward round, with a very slight deviation from perfect circularity. The core exhibits a yellowish-orange hue, suggesting an older stellar population dominated by redder giants and dwarfs. This central region gradually diffuses outward into a bluer halo. The absence of well-defined spiral arms or prominent dust lanes indicates a lack of significant recent star formation within a disk-like structure, which could potentially indicate it is an Elliptical galaxy. There are subtle hints of minor disturbances in the galaxy's outskirts, possibly indicative of a past or ongoing interaction with a smaller companion galaxy. The overall color profile indicates a moderate redshift, corresponding to a substantial distance and lookback time.
