The galaxy appears to be an elliptical galaxy, characterized by its generally smooth and featureless morphology. It exhibits a bright, concentrated central bulge that diminishes gradually toward the outer edges, suggestive of an older stellar population. There are no apparent spiral arms or dust lanes. The galaxy's shape is generally round, exhibiting a slight degree of ellipticity, falling somewhere between round and oblong. There is no visual evidence of any ongoing mergers or tidal disturbances suggesting a relatively stable, isolated system. The galaxy exhibits a yellowish hue, consistent with older stars which produce less blue light than younger stars. The outer halo seems to fade out gradually.
