The galaxy presents as a fairly smooth, centrally concentrated object with a rounded morphology. Its core exhibits a bright, yellowish-white hue, suggestive of an older stellar population. The light gradually diffuses outward from the center, transitioning into a dimmer, more reddish-toned halo. The smoothness of the light distribution is suggestive of an elliptical galaxy, with the absence of clearly defined spiral arms or a prominent disk structure. There might be a slight disturbance in its shape, but overall, the galaxy does not seem to be undergoing any major merging activity. The galaxy's apparent size is relatively compact.
