The galaxy presents as a somewhat elliptical, concentrated structure. The central region exhibits a bright, yellowish hue, suggestive of an older stellar population. Proceeding outward, there is a less defined disk component.

Based on the observed colors, there is some ongoing star formation activity, although likely at a modest rate. There do not appear to be any prominent spiral arms or bars. Its morphology suggests a relatively undisturbed system, with no obvious signs of a major merger event. The shape is tending to be considered somewhere between round and elliptical.
