The galaxy presents as an elliptical morphology, though displaying a slight disk-like feature. The central bulge is bright and concentrated, exhibiting a yellowish-white hue suggestive of an older stellar population. Moving outward, the galaxy fades into a blueish halo, indicating a potential, albeit weak, presence of more recent star formation in the outer regions. There are no prominent spiral arms or distinct dust lanes visible. The galaxy appears relatively smooth, with no major signs of ongoing mergers or significant tidal disturbances, although a slight distortion could suggest a minor gravitational interaction in the past or present. The red shift indicates this object is relatively distant, thus many details are difficult to resolve.
