The galaxy presents a generally smooth morphology, suggestive of an elliptical or lenticular type. It exhibits a bright, centrally concentrated core that fades into a diffuse halo. The galaxy appears to be elongated, but only slightly. There are no prominent spiral arms or bar structures visible. There is a subtle color gradient within the galaxy, transitioning from a bluer hue in the central region to redder tones in the outskirts. There is no evidence of any major merger events, although a slight disturbance or minor interaction cannot be completely ruled out.
