The galaxy appears as an elliptical-type, with a smooth, concentrated light profile. The core of the galaxy exhibits a bright, yellowish-white hue, indicating a likely older stellar population. Moving outward from the core, the galaxy gradually transitions to a fainter, reddish-orange color, implying a decline in ongoing star formation in the outer regions. The overall shape is somewhat elongated, with no obvious signs of spiral arms or a prominent disk. There are hints of minor disturbances in the morphology, possibly suggesting past or ongoing interactions, although a major merger is not apparent. The galaxy appears relatively isolated in this field of view.
