The galaxy presents as a centrally concentrated object with a smooth, diffuse morphology. The central region exhibits a bright, prominent core, indicative of a high stellar density.  The light profile appears to fade gradually from the core outward, lacking any distinct spiral arm structure or other features associated with disk galaxies. The overall color is slightly reddish-yellow, potentially suggesting an older stellar population and a relatively low rate of ongoing star formation. There is little evidence of tidal disturbances or interactions with other galaxies in the immediate vicinity. The shape is somewhat elliptical, though deviates only slightly from being perfectly circular.
